The galaxy presents as a somewhat elliptical, relatively smooth structure, exhibiting characteristics suggestive of a transitioning morphology between a spiral and elliptical galaxy. The central bulge is bright and concentrated, gradually fading outwards into a less defined disk. Some asymmetry is apparent, possibly indicating minor tidal disturbance or interaction with another galaxy in the past, though no distinct companion galaxy is readily visible in this image.

Color variations are subtle. The central region displays a yellowish-white hue, likely indicative of an older stellar population. A bluer tint is visible in the outskirts, potentially suggesting ongoing star formation in that region. This galaxy exhibits weak star formation and is a moderate mass galaxy.
