The galaxy presents a generally smooth and featureless morphology, indicative of an elliptical or lenticular type. Its shape appears to be mostly round, with only a slight deviation towards an elongated form. There is a distinct central bulge exhibiting the brightest and most concentrated luminosity. The color profile suggests a population of older stars, contributing to the galaxy's reddish-yellow hue. While there are some subtle color variations, the overall distribution appears relatively uniform, lacking prominent spiral arms or dust lanes. There is no obvious visual evidence of ongoing major mergers or significant tidal disturbances. Subtle minor disturbances or interactions cannot be ruled out. The overall impression is of a fairly mature, quiescent system.
