The galaxy presents as a somewhat elongated, elliptical-like structure. It exhibits a smooth, diffused appearance with no readily discernible spiral arms or distinct features. A bright, concentrated central bulge is visible, surrounded by a fainter, more extended halo or disk component. The overall color appears to be predominantly yellowish-orange, suggesting an older stellar population. There may be a slight hint of blue tint in the outer regions of the galaxy, which could be indicative of some recent or ongoing star formation, but it could also be artifact. No strong evidence of tidal disturbances, major mergers, or active galactic nuclei (AGN) activity is immediately apparent.
