The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge exhibiting a yellowish hue. A faint, diffuse halo surrounds the brighter core, gradually fading into the background. There is no prominent disk-like feature or spiral arm structure visible. The overall shape is approximately round, with only a slight deviation toward an elongated form. There is no readily apparent evidence of ongoing major merger events, although subtle irregularities may suggest minor disturbances or tidal interactions. The observed color gradient suggests a stellar population dominated by older stars, with a low rate of ongoing star formation.
