The galaxy presents a generally elliptical morphology, appearing elongated but lacking significant spiral arm structures. A bright, concentrated central bulge dominates the galaxy's core, exhibiting a yellowish hue suggestive of an older stellar population. The light appears to gradually fade towards the outer edges.

The disk component, though not clearly resolved into distinct arms, shows hints of blue in the outer regions, potentially indicating pockets of younger, hotter stars and ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. A slight asymmetry in the outer regions of the disk is present, but it is difficult to characterize further at this resolution.
