The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical and gradually fading into an extended halo. There's a slight elongation, deviating marginally from a perfect circle, but it does not appear cigar shaped. No obvious spiral arm structure or distinct dust lanes are visible. The overall color profile suggests a mature stellar population, with a relatively uniform yellowish-white hue indicative of older stars dominating the light output. There is no strong evidence of ongoing major mergers or significant tidal disturbances. There might be a slight asymmetry, but the overall impression is that of a relatively undisturbed system. The galaxy's light profile suggests a lack of recent, intense star formation activity.
