The galaxy presents as a moderately bright, relatively smooth elliptical or lenticular type. Its light profile appears centrally concentrated, with a gradual decline in brightness towards the outer regions. A slight elongation is visible, suggesting a deviation from a perfect sphere. The core region exhibits a yellowish-white hue, potentially indicative of an older stellar population. Fainter, bluer regions are subtly interspersed, possibly tracing younger stars. There are no prominent spiral arms or strong dust lanes visible. There is no evidence of any ongoing major merging events, but subtle disturbances are possible. The morphology is consistent with a galaxy of significant mass and moderate star formation rate.
