The galaxy presents as a moderately luminous, elongated structure. The central region exhibits a concentrated, smooth morphology, with a distinct yellow-orange hue, suggesting an older stellar population. Fainter, bluer light emanates from the outer regions, potentially indicative of ongoing or recent star formation. The overall shape appears transitional, possessing features of both elliptical and disk galaxies, though lacking a clearly defined spiral arm structure. There are minor visual disturbances present, but no strong indications of a major ongoing merger, though minor disturbances are visible. The galaxy's axial ratio suggests a significant inclination relative to our line of sight.
