The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with minimal discernible features. The core region displays a bright, concentrated luminosity profile, suggestive of a high stellar density or possible AGN activity, although no distinct nucleus is visually resolved. The color gradient appears relatively uniform across the galaxy, with a slight shift towards redder hues in the outer regions, possibly indicating an older stellar population. There is no apparent evidence of spiral arm structures, dust lanes, or significant star formation regions within the observed image. The overall shape approximates a sphere, with minimal ellipticity observed. No indications of tidal disturbances or ongoing merger activity are visually apparent; it is a rather regular shape.
