The galaxy presents as a slightly elongated object, seemingly smooth in texture with a diffuse profile, suggesting an elliptical morphology or a face-on spiral galaxy with a prominent bulge and weak spiral arms. The color is mostly uniform, and the galaxy's light is shifted towards the redder end of the spectrum. There are no obvious signs of active star formation regions or prominent dust lanes, indicating a likely older stellar population with a relatively low star formation rate. The galaxy appears to be relatively isolated. There may be a slight distortion in shape indicating a possible minor interaction with another galaxy.
