This galaxy exhibits a generally smooth morphology, appearing largely featureless in this observation. Its shape is highly circular, displaying a high degree of rotational symmetry. There is no visual evidence of strong tidal interactions or major disturbances affecting the overall structure. The galaxy shows a centrally concentrated luminosity profile, with a bright, yellowish core region that gradually fades into a dimmer, less defined outer halo. The color suggests a stellar population dominated by older, redder stars, indicative of a relatively low star formation rate. Subtle extensions might be present but are indistinct, perhaps indicative of minor accretion events. The overall impression is of a well-evolved, quiescent system.
