The galaxy presents a smooth, elliptical morphology with a notable central bulge. The light distribution appears concentrated, decreasing gradually from the core outwards. There is a slight elongation present, suggesting it is not perfectly spherical but rather somewhat cigar-shaped.  Color gradients indicate a dominant population of older stars, with a yellowish-red hue becoming more prominent towards the center of the galaxy.  There is no clear evidence of spiral arms, dust lanes, or other distinct features typically associated with disk galaxies. There's no indication of any major ongoing merger activity or significant tidal disturbances.  The galaxy appears relatively undisturbed and evolved.