The galaxy presents a generally smooth appearance, with a central bulge that is slightly elongated. The overall color profile suggests a population dominated by older stars, yet there is a green presence in the galaxy implying areas of active star formation. While the galaxy is mostly smooth, there appears to be a slight asymmetry or minor irregularity in its outer regions, possibly indicating a past or ongoing minor interaction. No distinct spiral arms or bar structure are apparent. The galaxy's shape is neither perfectly round nor highly elongated, appearing somewhat elliptical. Overall, the galaxy appears to be relatively undisturbed, with no major merging events visibly distorting its structure.
