The galaxy appears to be a relatively compact object with a noticeable central bulge. There is a faint suggestion of a spiral arm structure, or potentially a disk-like structure viewed at a high inclination. The color profile suggests the presence of a slightly older stellar population, as it appears somewhat redder in color. There might be some faint indications of minor tidal disturbances or interactions. The galaxy may be experiencing a minor interaction with a very faint object, but more data would be required for confirmation.