The galaxy presents a generally smooth morphology, exhibiting a high degree of radial symmetry. Its shape is predominantly round. There appears to be a concentration of light towards the galactic center, suggesting a central bulge. Fainter, diffuse light extends outward from this central region. The galaxy's color profile is primarily red, possibly indicating an older stellar population, though bluer hues can be observed in areas outside the bulge, suggesting some ongoing star formation. There does not appear to be any evidence of a major merger or significant tidal disturbances in its structure. Some possible minor disturbances in the morphology are possible, but the galaxy is mostly undisturbed.
