The galaxy presents as a diffuse, disk-like structure, though the resolution limits detailed morphological classification. The light distribution appears relatively smooth, exhibiting a central concentration that suggests a bulge component. There are no distinct spiral arms or bar features readily apparent. The galaxy's color profile indicates a significant population of older stars, contributing to a reddish hue. There may be some signs of mild gravitational disturbance. However, no significant merger events or tidal tails are readily visible. Overall, the galaxy presents as a relatively undisturbed system, dominated by older stellar populations, with a smooth appearance.
