The galaxy presents a moderately bright central bulge, suggesting a substantial concentration of older stars. The morphology is somewhat ambiguous; while it displays a relatively smooth overall appearance, there's evidence of a disk-like structure extending outwards from the bulge. The galaxy exhibits a subtle blue hue, particularly in the disk region, indicative of ongoing star formation, though not at an exceptionally vigorous rate. The overall shape is elongated, not perfectly spherical, with a tendency towards an intermediate elliptical form. There might be minor disturbances or asymmetries in the outer regions of the galaxy, hinting at possible past interactions or mergers, but no clearly defined tidal tails or significantly disrupted features are apparent. Overall, it appears to be a galaxy transitioning between a spiral and elliptical morphology, with moderate star formation activity and a possibility of past interactions influencing its current structure.
