The galaxy presents as an elliptical or lenticular system. Its overall color is a pale yellow. There is a brighter, more intensely yellow central bulge or core, surrounded by a less intensely colored halo of similar hue. The galaxy appears to be elongated, suggesting it is not spherical but more cigar shaped. There are hints of a flattened disk structure within the halo region, but no spiral arms are apparent.  The outer edges are smooth and diffuse, though there are subtle asymmetries that might indicate minor gravitational interaction or internal disturbances. There is no strong evidence of ongoing major merger activity.  Based on the color profile, it is likely composed primarily of older stellar populations.
