The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The light profile appears to gradually fade from the core outward, lacking distinct spiral arm features. The color gradient suggests a population of older stars dominating the light emission, with a possible enhancement of slightly younger stars toward the central region. There is no visual evidence of significant dust lanes or active star formation regions. The overall structure appears undisturbed, showing no signs of recent mergers or tidal interactions.
