The galaxy appears to be a spiral galaxy, likely somewhere between a lenticular (S0) and a more open spiral type. It presents a generally smooth appearance, with a bright, concentrated central bulge that dominates the luminosity. The galaxy has an elliptical shape with an aspect ratio that suggests it is being viewed at a significant inclination. The spiral arms are not well-defined; instead, there is a somewhat diffuse disk component.

The overall color of the galaxy is somewhat blue in the outer regions, potentially indicating recent or ongoing star formation. The central bulge appears yellower, consistent with an older stellar population. There is no prominent dust lane visible and no obvious signatures of ongoing merger activity, although there may be some minor disturbances in its morphology. The light is concentrated towards the center. The galaxy has a substantial mass, given its luminosity and inferred star formation rate.
