The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The luminosity appears to be highest at the core, gradually decreasing outwards. There's a subtle color gradient across the galaxy, with the central region exhibiting a yellowish-white hue that transitions to redder tones in the outer regions. This color suggests an older stellar population in the core, consistent with reduced star formation activity. There's a possible minor disturbance or feature visible as an extension, or separate entity, near one edge of the galaxy. Overall, the galaxy appears relatively isolated and undisturbed, with no clear signs of a major ongoing merger or significant tidal interactions.
