The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse structure. A concentrated central bulge is apparent, with a gradual decrease in luminosity towards the outer regions. The overall color profile suggests a relatively older stellar population, exhibiting a yellowish-red hue concentrated in the core with cooler, blue-shifted regions around the perimeter of the galaxy. The general shape is somewhat elongated with the ratio between the major and minor axes indicating a mild flattening. There appears to be minimal presence of dust lanes or active star-forming regions within the galaxy. Overall, the galaxy shows no obvious signs of major interactions or recent mergers.
