The galaxy appears as a diffuse, moderately sized object with a relatively smooth morphology. The color profile suggests a higher concentration of older stellar populations, with a general reddish-orange hue dominating the overall light emission. There are subtle indications of slight distortions or faint tidal features, potentially indicative of minor gravitational interactions or past merger events. The central region appears slightly brighter, possibly containing a bulge component. Overall, the galaxy exhibits characteristics of a late-type spiral galaxy, but lacking distinct spiral arm structures.
