The galaxy appears as a somewhat elongated, elliptical-like structure. Its color profile suggests a substantial population of older stars, exhibiting a yellowish-red hue. There is little to no evidence of distinct spiral arm structures or prominent dust lanes. The light is concentrated towards the center, implying the presence of a central bulge. The overall smoothness of the light distribution indicates that the galaxy is likely an early-type galaxy with minimal recent star formation activity. The galaxy's shape indicates that is is not very round, and more cigar shaped. The morphology suggests that the galaxy is not undergoing a major merger or significant tidal disturbance.
