The galaxy presents as an elliptical morphology. It appears relatively smooth in structure with a moderate ellipticity, tending towards a somewhat rounded shape, though not perfectly circular. The color profile indicates a dominant redder population of stars, with the bluer light relatively suppressed. This suggests that it is a quiescent galaxy with relatively little ongoing star formation and comprised of an older stellar population. There is no obvious evidence of spiral arms, a central bar, or significant dust lanes. There are no indications of any major ongoing merger events or strong tidal disturbances in the galaxy's morphology. The lack of significant bluer regions points away from strong starburst activity.
