The galaxy appears to be relatively smooth, with a somewhat elliptical morphology. A slight central bulge is visible, although it is not highly pronounced. There is evidence of a disk component, but it is not strongly defined; the spiral arms, if present, are tightly wound and not easily discernable. The overall color profile suggests a population of older stars, with a generally redder hue that indicates relatively low star formation activity. There are some indications of minor disturbances, potentially suggesting a past or ongoing interaction with another galaxy, or perhaps internal dynamic processes. The object is somewhat elongated, but is mostly rounded. There are low indications of recent merging events.
