The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a yellow-white hue, indicative of an older stellar population. There are hints of a fainter, diffuse halo surrounding the central region, showing a slightly greenish tint perhaps indicating some low level of ongoing star formation. The overall shape suggests an intermediate form, neither perfectly spherical nor elongated into a cigar shape. There is a nearby object to the right that may be undergoing a slight disturbance or merger, but this may simply be a case of visual superposition. The galaxy does not show strong evidence of spiral arms or a well-defined disk structure. Overall, the appearance suggests a relatively massive galaxy with a subdued star formation rate, consistent with a later stage of galactic evolution.
