The galaxy presents as a relatively compact object, exhibiting a general spheroidal morphology. The light distribution appears smooth and centrally concentrated. There is evidence of faint, extended features surrounding the central region, potentially indicative of tidal interactions or previous merger events. The galaxy appears slightly elongated, deviating somewhat from a perfectly circular profile. The color profile suggests a population of older stars, with a noticeable redder hue in comparison to galaxies with ongoing active star formation. The object shows characteristics of a massive galaxy, potentially a lenticular or elliptical type. There is a possibility of some minor disturbances of the galaxy's morphology, but it's overall structure is relatively undisturbed. There are no apparent spiral arm structures visible in this image. 
