The galaxy presents as a somewhat elongated, lenticular or possibly spiral system viewed at an oblique angle. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. Fainter, blue-tinged diffuse regions extend from the central area, likely indicating areas of more recent star formation within the galaxy's disk. The overall structure appears somewhat disturbed, with faint trailing edges, possibly suggesting past or ongoing interactions with another galaxy. There is a component of smoothness to this galaxy, but there are features indicating disturbance within the disk of the galaxy. The galaxy shows an intermediate rounded shape with a relatively low rate of star formation. Finally, there is evidence that this galaxy may be merging.
