The galaxy presents as a relatively smooth, elliptical structure, appearing nearly circular in projection. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. A subtle color gradient is discernible, transitioning from a redder hue in the central region to slightly bluer tones in the outer halo. There is no obvious dust lane or prominent spiral arm structure indicative of ongoing active star formation on a large scale. Minor disturbances are not easily discerned, which supports the possibility of it being a relaxed system. Overall, the galaxy appears to be a quiescent system with minimal recent merger activity.