The galaxy appears as a single, concentrated body of light, with a mostly homogenous structure. It exhibits a smooth, elliptical morphology, without prominent spiral arms or a discernible disk. The galaxy's color profile suggests a population of older stars, given the redder hues. It is highly round in shape. There is no apparent active galactic nucleus or significant dust lanes, further supporting the hypothesis of an older stellar population and a lack of ongoing major star formation. There is no major disruption present that would point to any significant mergers or tidal interactions.
