The galaxy presents as a generally smooth, elliptical-like structure. There is a high degree of central concentration, with the light intensity gradually decreasing outwards. The galaxy appears largely featureless, with no apparent spiral arms or bar structures. The overall color profile seems to be a yellow-orange hue, suggesting a population of older stars. There may be minimal ongoing star formation, with evidence of older stellar populations dominating the luminosity. There is no obvious evidence of tidal disturbances or mergers, with a fairly relaxed and symmetric morphology.
