The galaxy presents a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile with a general lack of distinct spiral arm structures or prominent dust lanes. The color gradient suggests a potential redder core region, possibly indicative of an older stellar population or increased dust obscuration toward the center. Fainter bluish halos are visible, which potentially indicate more recent star formation in the outskirt regions. Close visual inspection of the galaxy does not reveal obvious major merging features or significant tidal disturbances, though the outer edges of the galaxy look slightly irregular. The galaxy appears round.
