The galaxy presents an elliptical morphology, appearing as a somewhat diffuse object with a concentrated central bulge. There is a subtle asymmetry in its overall shape, suggesting possible tidal interactions or minor disturbances. The color profile indicates a stellar population that is primarily intermediate to old, with a noticeable lack of intense blue star-forming regions. The light distribution gradually decreases from the center outwards. The presence of possible minor mergers may be disrupting the galaxy's shape. The dust lanes are not clearly visible, indicating a lack of significant amounts of cold gas or dust. The structure seems to have a small disk.