The galaxy presents a generally smooth appearance with some discernible internal structure. Its overall shape is elliptical, exhibiting a moderate degree of elongation. The color profile indicates a redder hue, suggesting an older stellar population with fewer young, massive stars contributing to the overall light output. While the main body of the galaxy appears relatively undisturbed, there is faint evidence of tidal features or minor disturbances in its outer regions, potentially indicative of a past or ongoing interaction with another galaxy. The galaxy's luminosity suggests that it is a massive system.
