The galaxy presents a morphology consistent with that of an elliptical or lenticular galaxy. It exhibits a smooth, centrally concentrated luminosity profile, with a shallow gradient moving outwards from a bright core. The overall shape is elongated, indicating a degree of flattening. The galaxy displays a yellowish-white hue, suggesting an older stellar population. There are no visible spiral arms or prominent dust lanes. Faint blue-ish regions can be observed around the central nucleus, possible areas of star formation. There is no apparent evidence of major mergers or tidal disturbances.
