The galaxy exhibits a morphology characterized by a predominantly smooth appearance. It has an approximate angular diameter of 2.8 arcseconds. There is a concentrated central bulge exhibiting a greenish-yellow hue, indicative of a population of older stars or potentially significant dust extinction. Surrounding the bulge is a more diffuse, blueish halo. This halo may be indicative of a younger stellar population undergoing active star formation. However, there are no immediately discernable spiral arm structures or other distinct features. The overall shape appears roughly elliptical. Some minor disturbances may be occurring, or perhaps the galaxy is a recent merger. Overall, the galaxy appears to be in a relatively late stage of its evolution.
