The galaxy presents a generally smooth morphology, with a central bulge that appears yellow-white, indicating an older stellar population. The galaxy exhibits a discernible disk structure, though the disk appears relatively featureless. The disk extends outward from the bulge and is bluer in color, suggestive of ongoing star formation. Overall the galaxy appears to be relatively isolated. The overall shape is somewhat flattened and spheroidal. The galaxy displays a slight blue hue, consistent with a moderate level of ongoing star formation. There is no sign of spiral arms, and there is no indication of any major mergers or tidal disturbances.
