The galaxy presents as a compact, elliptical structure. It exhibits a smooth, relatively featureless morphology with no readily discernible spiral arms or bar. The light distribution appears concentrated towards the center, with a gradual decline in luminosity towards the outer edges. The galaxy's color profile suggests an older stellar population, displaying a yellowish-red hue characteristic of evolved stars. There is no evidence of significant dust lanes or recent star formation activity within the visible portion of the galaxy. The overall impression is that of a well-formed, relaxed galaxy, likely devoid of any ongoing major mergers or significant interactions.
