The galaxy presents as a largely featureless, elliptical morphology. It exhibits a concentrated central bulge with a smooth, diffuse halo extending outwards. The color gradient suggests an older stellar population, with the central region appearing more yellow, potentially indicating a higher concentration of evolved stars. There is a subtle decline in brightness from the core outwards, with no apparent spiral arms or dust lanes visible. The overall structure implies a system that is likely dynamically relaxed, consistent with an elliptical classification. There are no signs of ongoing major mergers or tidal disturbances, although subtle irregularities in the outer halo cannot be entirely ruled out at this resolution. Given the smoothness and roundness, this galaxy appears to be approaching a spheroidal shape.
