The galaxy appears to be an elliptical-type galaxy, exhibiting a generally smooth morphology. The central region is characterized by a bright, concentrated luminosity, indicative of a dense stellar population or potentially an active galactic nucleus. The isophotes appear to be relatively round. There is some evidence of tidal disturbances or interactions, manifested as faint streams or extensions of light emanating from the main galactic body, predominantly towards the upper left of the image. The overall color profile suggests a mix of stellar populations, with redder hues dominating the central bulge and bluer tints appearing in the outer regions, potentially signaling younger stars or ongoing star formation in those areas. There also is a secondary nucleus or a smaller galaxy appears to be interacting with the main galaxy, contributing to the observed distortions and tidal features. The galaxy exhibits an estimated redshift of z ~ 0.34, implying a substantial distance and lookback time. Overall, the galaxy presents as an intermediate-mass system currently undergoing or having recently undergone a merger event.
