The galaxy presents as a relatively smooth, elliptical morphology with minimal discernible substructure. The light distribution appears centrally concentrated, exhibiting a gradual decrease in intensity outwards from the nucleus. The color profile suggests an older stellar population, with a dominant yellowish-red hue indicative of evolved stars. There is no evidence of significant spiral arm structure, or dust lanes. The overall roundness of the galaxy is pronounced, lacking any obvious elongation or tidal features that would suggest recent or ongoing interactions with other galaxies. Faint, extended emission may be present in the outer regions, although this is difficult to ascertain definitively due to the image's resolution. The estimated physical size indicates it is a substantial galaxy. The galaxy appears to be at moderate redshift. Overall, the galaxy likely is a massive early-type galaxy with a relatively low star formation rate.
