The galaxy presents as an elliptical morphology, appearing generally smooth in texture. It exhibits a concentrated central bulge that transitions gradually outwards. The color profile appears relatively uniform across the galaxy, with a slight shift towards redder hues in the central bulge. No prominent spiral arm structures, dust lanes, or irregular features are clearly discernible in this observation. Based on its overall structure and color, this galaxy likely hosts a population of older stars, with reduced recent star formation activity.