The galaxy presents an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core exhibits a yellowish-white hue, suggesting a dominant population of older stars. The galaxy's overall color appears to be redder than bluer, implying a relatively quiescent state with suppressed star formation activity. The galaxy appears elongated, with a major axis significantly longer than its minor axis, exhibiting a moderate flattening. There are no readily apparent spiral arm structures or dust lanes visible. There also appears to be some minor disturbance due to a possible merging event.
