The galaxy presents as an elliptical morphology, elongated in shape. The light distribution appears relatively smooth and centrally concentrated, with a notable lack of discernible spiral arms or distinct features such as dust lanes or star-forming regions. There is a color gradient from the center outwards, displaying a yellow-white central bulge which could mean it contains older stellar populations. There is no apparent ongoing major merger activity or significant tidal disturbances, implying it is relatively isolated in its environment. However, the fuzziness of the outer edges, and the subtle irregularities in its shape could indicate some minor tidal effects, perhaps the result of minor disturbances.
