The galaxy appears as a lenticular or possibly an elliptical type. Its morphology is smooth, with no distinct spiral arms or prominent features readily apparent. The shape is elongated, possibly cigar-shaped, suggesting a non-spherical distribution of stars. There is no clear indication of a recent major merger event or significant tidal disturbances based on its overall structure. The galaxy exhibits a slightly bluer hue at its edges and a more pronounced red/yellow central bulge indicating a more established stellar population in the core and a younger stellar population in the disk/outer edges.
