The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. It exhibits a bright, yellowish core, suggestive of an older stellar population, with light decreasing in intensity further away from the center. There is a faint disk structure that is subtly bluer in color, which could indicate the presence of more recent star formation within the disk. There is little evidence of any significant disturbances or tidal features, indicating that the galaxy is likely not currently undergoing a major merger. The overall appearance suggests this is a massive galaxy with a well-defined structure and a mix of stellar populations.
