The galaxy presents as a somewhat elliptical object, with a concentrated central bulge exhibiting a yellow-orange hue. The surrounding galactic disk appears less defined, showing a mottled texture with hints of blue and green, potentially indicating regions of active star formation. The galaxy appears generally smooth, although there is an apparent minor distortion on one side, potentially indicative of a previous or ongoing minor interaction with another galaxy. The overall color profile suggests a significant population of older stars within the central region, with a comparatively younger stellar population present in the disk. There is no evident spiral arm structure. The galaxy appears to be relatively isolated.
