The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure with no apparent spiral arms or prominent dust lanes. Its color profile indicates a dominant population of older stars, evidenced by the reddish-gold hue. The galaxy appears relatively isolated, lacking any significant signs of tidal interactions or merging events. A slight elongation is discernible in its overall shape, suggesting a possible deviation from a perfectly spherical structure. The overall light distribution is centrally concentrated, typical of elliptical galaxies.
