The galaxy presents a generally elliptical morphology, with a smooth, featureless appearance. The central region exhibits a concentrated brightness, suggesting a high stellar density, potentially indicative of an older stellar population. The color of the central bulge is predominantly yellowish-orange, consistent with evolved stars. Moving outwards from the center, the color gradient shifts toward a slightly bluer hue in the outer regions of the galaxy. This suggests the presence of younger, hotter stars and potentially ongoing star formation, although this activity appears to be at a subdued level overall. There is no strong evidence of spiral arm structures, bars, or significant dust lanes within the visible light image, suggesting a relatively relaxed dynamical state, with only minor disturbances and no major mergers apparent. The overall shape tends to be in between round and cigar shaped, slightly more rounded.
