The galaxy presents as a relatively smooth, elliptical-like structure. There are no readily apparent spiral arms or a distinct disk component. The light distribution appears centrally concentrated, gradually fading outwards, suggesting a high degree of symmetry. The color profile shows a slightly redder core, indicative of an older stellar population dominating the central region. The overall smoothness suggests it may be an early-type galaxy, likely an elliptical or lenticular galaxy. There may be a slight asymmetry to the galaxy's halo but this may be due to instrument error. There are no visible signs of active galactic nuclei, nor are there any nearby galaxies or galaxy tidal tails to suggest a recent merger event. 
