The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth and rounded morphology. The central region displays a bright, compact core. A slightly flattened spheroid structure, likely a bulge, surrounds the nucleus, showing a gradual decrease in luminosity outwards. The overall color of the galaxy is slightly blue, indicating the presence of a young stellar population and ongoing star formation, even if at a low rate. There are no prominent spiral arms or other features typically associated with late-type galaxies. There is some indication of slight disturbance of asymmetry, but no conclusive evidence of major mergers or tidal interactions.
