This galaxy presents as a somewhat elongated, lenticular-like structure. Its light profile suggests a centrally concentrated bulge region that gradually fades outwards towards a diffuse, extended disk. The color distribution is relatively smooth across the galaxy. The central bulge appears to be slightly bluer than the outer regions of the disk, but the disk overall has some blueness. There is also a suggestion of possible minor tidal disturbance or ongoing merger activity based on slight irregularities. The morphology of the galaxy exhibits characteristics of a spiral or an elliptical galaxy, and based on the general rounded profile of this object, it may be closer to an elliptical. There appears to be a very faint disk around the galaxy. There does not appear to be strong evidence of ongoing star formation, but there may be some.
