The galaxy presents as an elliptical morphology, with an overall smooth appearance. The central bulge exhibits a concentrated, bright luminosity, shifting towards a yellow-white hue. The outer regions of the galaxy display a gradual fading in intensity. There is a slight suggestion of a flattened shape. The galaxy appears relatively isolated with no evident tidal features or nearby companions indicative of recent major merger activity, although minor disturbances cannot be ruled out based on the current data. There is an absence of distinct spiral arm structures or prominent dust lanes. The color profile suggests a population of older stars and a low rate of current star formation activity.
