The galaxy appears to be a relatively smooth, elliptical type galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The galaxy displays a slight elongation and a subtle disk-like feature. The color profile suggests the presence of an older stellar population, with a more pronounced concentration of older stars. There's a hint of faint, diffuse bluer regions within the galaxy, suggestive of possible localized areas of ongoing star formation. No significant dust lanes or prominent spiral arm structures are apparent. Overall, the galaxy appears to be in a relatively quiescent state.
