The galaxy presents as a relatively smooth, elliptical morphology, with a concentrated central bulge that dominates its overall structure. The color appears generally redder, particularly within the central region, indicative of an older stellar population and a diminished rate of star formation. There is some indication of a faint, diffuse halo surrounding the central region, though the boundaries are not well-defined. A small, slightly bluer region is visible at one end of the galaxy, hinting at a possible region of ongoing star formation, however minimal. Overall, the galaxy appears evolved, likely characterized by a substantial stellar mass and a quiescent state in terms of star-forming activity. There may be some evidence of past gravitational interactions given the slight disturbances in the halo.
