The galaxy appears as a centrally concentrated object, displaying a radial brightness profile that decreases outwards from a bright, yellowish core. The main body of the galaxy is largely smooth in appearance. There is a slight elongation, but the overall form is generally round. Faint, diffuse extensions are visible surrounding the core, suggesting an extended halo or envelope of stars and/or dust. No distinct spiral arm structure or prominent dust lanes are readily discernible. The galaxy exhibits a color gradient, with the central region appearing yellower than the outer regions, which seem to have a hint of bluer components. Based on its morphology, it is likely an elliptical galaxy. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. However, a possible subtle asymmetry in the outer regions might indicate a minor interaction or past merger event.
