The galaxy presents a smooth, elongated morphology. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population likely dominated by evolved stars. Extending outwards from the bulge are fainter, bluish regions, possibly indicative of ongoing, albeit subdued, star formation within a disk structure. There is no apparent dust lane visible, nor any prominent spiral arm structure discernible in the image. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal interactions. Overall, this galaxy gives the impression of being a relatively evolved system with a moderate stellar mass and low specific star formation rate, resembling a lenticular or early-type spiral galaxy viewed at a significant inclination.
