The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The galaxy appears to be generally round. There is no evident spiral arm structure or distinct dust lanes. The color profile suggests a population of older stars, giving it a yellowish-red hue. No significant signs of ongoing major mergers or tidal disturbances are detected. A possible minor disturbance can't be ruled out with certainty.
