The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an elliptical morphology with a high degree of radial symmetry, appearing neither particularly flattened nor elongated. The core region shows a bright, concentrated luminosity profile, fading gradually towards the outer edges. The color distribution is not uniform, with a central region displaying warmer hues, possibly indicative of an older stellar population. Subtle variations in color are visible, potentially suggestive of variations in stellar populations or dust distribution within the galaxy. There is no obvious spiral structure, bar, or significant dust lane visible. Overall, the galaxy appears undisturbed, showing no signs of ongoing major mergers or tidal interactions. It is a likely candidate for an early-type galaxy, with little evidence of active star formation.
