The galaxy presents an overall smooth morphology with a predominantly elliptical shape. There is evidence of a bright central bulge that appears yellowish in color, suggesting a population of older stars. The light from the bulge gradually fades outward into a less defined disk. Some subtle asymmetry can be detected, however no distinct spiral arms or bar structures are visible. There are no prominent dust lanes. The galaxy appears to be relatively isolated, with no obvious signs of interaction with other galaxies, although subtle disturbances indicate that a recent merger may have occurred.
