The galaxy presents as a single, relatively smooth object with a concentrated central bulge. It is generally elliptical in shape, appearing largely rounded with minimal deviation from circularity. The galaxy exhibits a strong, bright core that diminishes in intensity towards its outer edges. Color gradients suggest an older stellar population, particularly evident in the central region which has a distinct yellow/red hue, indicative of evolved stars. There is no obvious presence of spiral arms or prominent dust lanes. The overall structure suggests a relatively undisturbed system, lacking strong indications of ongoing merger activity. Star formation rate appears low, correlating with the redder color of its stellar population.
