The galaxy presents as a somewhat elongated, disk-like structure with a prominent central bulge. The bulge region exhibits a bright, concentrated luminosity, suggesting a high density of stars. Moving outward from the bulge, the disk appears relatively smooth and lacks well-defined spiral arm structures. The overall color profile indicates a relatively older stellar population. Fainter extensions are present at the galaxy's extremities, possibly representing the outer reaches of the galactic disk. There are no clear signs of ongoing major merging activity or significant tidal disturbances within the visible structure. A subtle color gradient is observed, transitioning from a yellower core to slightly bluer outer regions, which may indicate some level of star formation within the galaxy. The galaxy's morphology leans towards a smooth disk galaxy, however, some irregularities do exist in the galaxy's disk shape and light profile.
