The galaxy presents an overall smooth morphology. The shape is elongated, with the ratio of the major to minor axis appearing significant. There appears to be a central bulge, though it lacks defined structure. There is little to no evidence of spiral arms or a prominent disk. The color profile suggests a population of older stars. No major mergers appear to be present. Some minor disturbances in the galaxy's profile may indicate a past or ongoing interaction, but they are not immediately evident from the image. The overall mass of the galaxy seems substantial. It appears that the star formation rate is low, and the galaxy may be transitioning to a more quiescent state.
