The galaxy presents as a relatively smooth, single structure. It has a concentrated central bulge, which dominates the galaxy's overall luminosity profile. The disk, if present, appears subdued.

The galaxy is approximately circular in shape, with only slight deviations from perfect symmetry. No strong tidal features or morphological distortions are apparent, suggesting it is unlikely to be undergoing a major merger event. There might be some minor disturbance on the edges of the galaxy.

In terms of color, the galaxy displays a yellowish-green hue, suggesting a moderate population of older stars. The outer regions appear redder, likely due to a slightly older stellar population. The overall color suggests the presence of a relatively low amount of on-going star formation within the galaxy.
