The galaxy appears as a centrally concentrated object with a diffuse halo. The light profile suggests a relatively smooth distribution, transitioning gradually from a bright core region to a fainter extended envelope. The shape of the galaxy is generally elliptical, with the semi-major and semi-minor axes being approximately equal. There is no strong indication of spiral arm structure or a prominent central bar. Subtle color variations are visible, with the core region exhibiting a slightly bluer hue compared to the outer regions, implying potential differences in stellar populations or dust content. There are no obvious signs of major tidal interactions or disruptions. A very subtle asymmetry is present, though this could be due to noise. Overall the galaxy exhibits the characteristics of an elliptical morphology.
