The galaxy presents as a relatively smooth, elliptical-like structure, with an observed elongation that is neither perfectly spherical nor highly flattened. The core region exhibits a brighter, more concentrated luminosity, suggesting a higher density of stars in that area. There is a subtle colour gradient across the galaxy, with the central region appearing slightly bluer compared to the outer edges, which trend towards redder hues. This could indicate a younger stellar population in the core or potential ongoing star formation. No distinct spiral arms or bar structures are readily apparent in this image; this is indicative of a galaxy with limited recent interaction or mergers. There may be minor perturbations within the galactic disk. Overall, the galaxy appears to be a relatively evolved system with characteristics of late-type spiral or early-type elliptical galaxies.
