The galaxy presents as a lenticular or possibly early-type spiral, viewed at a significant inclination. It exhibits a distinct, elongated morphology with a bright, concentrated central bulge. The bulge appears yellowish-white, suggesting an older stellar population. Surrounding the bulge is a fainter, bluer disk or halo. This disk appears smooth and lacks the prominent spiral arm structures or dust lanes typically associated with actively star-forming galaxies. The edges of the disk fade gradually into the background sky. There is some asymmetry in the outer regions, suggesting the possibility of minor tidal interactions, though no obvious signs of a major merger are readily apparent. The overall color profile indicates a relatively quiescent galaxy with a low star formation rate.
