The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a concentrated central bulge that gradually diffuses outwards into a less dense halo. The dominant color is yellowish-orange, suggesting a population of older stars with lower rates of ongoing star formation. The overall shape is mostly round, with minimal disk-like features or spiral arm structures visible. There is very little indication of any major mergers or significant disturbances in the galaxy's structure. A subtle blue hue is observable, possibly indicating a small degree of recent star formation.
