The galaxy presents as a single, somewhat amorphous body with an approximate radius of 1.5 arcseconds. It exhibits a generally smooth morphology, with a slight central concentration of light. There is subtle evidence of an asymmetric structure, potentially indicative of past or ongoing gravitational interactions. A faint, extended halo of diffuse light surrounds the central region.

The color profile suggests the presence of an older stellar population, with a moderately red color. However, some bluer regions are visible, indicating possible areas of more recent star formation, though they do not dominate the overall color. There may be evidence of minor tidal features, and some potential signs of a recent merger event in the form of slight disturbances to its symmetry.
