The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a mostly rounded morphology, with only a slight elongation visible. The color profile suggests a population of older stars, with a hint of bluer light concentrated in the central region, implying some ongoing star formation activity. There is a possible tidal tail or disturbance. The galaxy's overall structure appears largely undisturbed, with no signs of a major ongoing merger, though subtle disturbances cannot be ruled out.
