The galaxy appears as a relatively compact, disk-shaped structure. The central bulge seems prominent, showing a gradual increase in luminosity towards the center. The disk component appears somewhat patchy with subtle variations in color, possibly indicating regions of varying stellar populations or dust obscuration. There is a possible faint, slightly asymmetric tidal feature or disturbance visible, suggesting it may have undergone a minor interaction with another galaxy or perhaps it is still settling into a stable configuration. The galaxy's overall color is moderately red, potentially indicative of an older stellar population and/or significant dust reddening. Star formation rate appears low.
