The galaxy presents as a flattened, disk-like structure with a moderate inclination relative to the observer's line of sight. It appears to be relatively smooth, with a diffuse distribution of light and a lack of prominent spiral arms. The color profile indicates a population of older stars, as the galaxy appears reddish. The morphology suggests a system that has likely undergone significant evolution and a period of star formation has ended. There is minor disturbance to the morphology, which could be caused by a past merger or tidal interaction. The shape is consistent with an elliptical or lenticular type, possibly a disk galaxy trending towards an elliptical morphology. The estimated size is approximately 7 kpc in radius, fairly large compared to other galaxies. 
