The galaxy presents as a slightly elongated spheroid with a concentrated central bulge that appears yellowish-white, indicative of an older stellar population. Fainter, diffuse blue light extends away from the core in opposite directions suggesting the presence of a flattened disk.

There are no clear spiral arm structures visible. The distribution of light is relatively smooth. No obvious signs of tidal disturbances or ongoing major mergers are evident. The overall morphology leans toward an early-type disk galaxy.
