The galaxy presents as a slightly elongated, lenticular-like structure. The central region exhibits a high surface brightness and a yellowish-white hue, suggesting an older stellar population dominating the core. Moving outwards from the center, the color transitions to a slightly bluer and fainter hue. This suggests the presence of a younger stellar population towards the outer regions, but to a much lesser extent. The overall morphology is smooth and lacks defined spiral arms or a distinct bar structure. There is no clear indication of ongoing major mergers or significant tidal disturbances, though some faint and subtle asymmetries in the outer regions cannot be completely ruled out as minor interactions. The galaxy appears relatively isolated within the observed field.
