The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. There is no obvious spiral arm structure or strong dust lane features visible. The color profile suggests a population dominated by older stars, with a possible hint of some bluer star formation activity in the central region, although this is subdued. The galaxy shows no distinct signs of a major ongoing merger, though there might be some minor asymmetry that could indicate a past or ongoing interaction. Overall, the light distribution appears fairly regular, suggesting a relatively relaxed dynamical state. Its size appears to be intermediate, neither extremely compact nor overly extended.
