The galaxy presents as a faint, relatively compact object. Its overall color appears somewhat redder, suggesting a population dominated by older stars, though this requires spectroscopic verification. The morphology is broadly elliptical, appearing somewhat elongated with a smooth light distribution. There is little evidence of spiral arms, significant dust lanes, or active star formation regions within this image, supporting the notion of an older stellar population. There may be a small irregular structure or tidal feature to one side. Further data is required to determine the precise classification and evolutionary state.
