The galaxy appears as a relatively compact object, exhibiting a somewhat smooth morphology, though there is some indication of disturbed features. There may be some indication of a faint disk, but the evidence is not strong. There are also features indicative of a possible minor merger or tidal disturbance in the structure of the galaxy. The galaxy is centrally concentrated with a diffuse halo. There is no strong evidence of a bright galactic nucleus. The galaxy's color suggests the presence of a relatively old stellar population, with a potential small amount of ongoing star formation.
