The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall color is somewhat blue-ish, suggesting the presence of a young stellar population. The central region exhibits a brighter concentration of light, possibly indicative of a bulge. The outer regions seem to fade gradually, with no distinct spiral arms or bar structures readily apparent. There are some subtle irregularities in the outer isophotes, possibly hints of minor tidal disturbances or interactions, although no significant merging event is immediately visible. Overall, the galaxy presents a somewhat elliptical morphology, but with hints of disk features. Star formation appears to be moderate within the galaxy.
