The galaxy appears as a single, centrally concentrated object with a smooth morphology. Its light profile exhibits a centrally dominant component that gradually fades outward without any obvious spiral arm structures or prominent dust lanes. The overall shape seems close to round. The color is relatively uniform, with a slightly yellowish hue, suggesting a stellar population dominated by older stars and a lack of significant ongoing star formation. There is no obvious distortion or tidal features indicating a recent major merger, but there may be some subtle asymmetry or minor disturbances within the central region. 
