The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The galaxy presents a generally rounded morphology, exhibiting a shallow radial surface brightness gradient. The core of the galaxy appears to have a yellow-white hue, possibly indicating an older stellar population. The outer regions of the galaxy display a slight falloff in intensity with increasing radius, suggesting a diminishing stellar density further from the center. There is a subtle indication of a possible minor disturbance in the galaxy's structure, such as a faint tidal tail or asymmetry, but more data is required to be conclusive. The galaxy does not appear to be actively merging.