The galaxy appears to be a relatively smooth, centralized object with a concentration of light toward the core. It presents as having an elliptical morphology, with a radial decrease in luminosity from the center outwards. The galaxy displays an overall yellowish hue, suggestive of an older stellar population dominating the light emission. There is little evidence of prominent spiral arms or significant dust lanes. A slight elongation is observed, but the galaxy is largely round in shape. No major signs of ongoing merging activity or significant disturbances are readily apparent, suggesting a system primarily relaxed and evolved. A slight asymmetry in the outer regions cannot be ruled out but overall there is nothing that stands out.
