The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated bulge region. The core exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, a slightly bluer, more diffuse halo is observed, possibly indicating ongoing or recent star formation. There is some indication of a possible tidal disturbance to the right side of the image, where the galaxy appears slightly elongated with some asymmetries. However, given the relatively smooth overall appearance, this could also be due to an interaction with another galaxy or a minor merger event in the past. The galaxy's overall shape is somewhat flattened but does not have a clear disk-like structure. The lack of prominent spiral arms or dust lanes further supports a classification towards the elliptical or lenticular end of the Hubble sequence.
