The galaxy presents a roughly elliptical morphology, appearing as a flattened spheroid when viewed from our vantage point. It exhibits a bright, concentrated central bulge, which appears yellow-white in color, suggesting an older stellar population with a relatively low rate of current star formation. 

Surrounding the bulge is a fainter, bluer disk. The blue color implies the presence of younger, hotter stars and ongoing star formation. Faint spiral arm structures are possibly present, although poorly defined, in the outer regions of the disk. The galaxy's overall structure appears relatively undisturbed, without significant signs of tidal interactions or recent major mergers, though minor disturbances are possibly present. A bar structure appears to not be present. The galaxy is viewed at an angle far from edge-on.
