The galaxy appears as a relatively smooth, elliptical structure with a slight elongation. Its core exhibits a concentrated luminosity, gradually fading outwards into a diffuse halo. There's a subtle color gradient, with the central region leaning towards a yellow hue, possibly indicating an older stellar population. No distinct spiral arms or prominent dust lanes are visible. Faint disturbances and asymmetry suggest a possible interaction in the past or present. The overall morphology indicates a system dominated by older stars.
