The galaxy presents as a single, somewhat amorphous object with a smooth light distribution. A distinct central bulge is observed with a yellowish hue, possibly indicating an older stellar population. There appears to be a diffuse, reddish component slightly offset from the central bulge which could indicate ongoing star formation or dust attenuation. The galaxy exhibits a generally elliptical shape, but with some noticeable disturbances or distortions in its outer regions. These disturbances may indicate minor gravitational interactions or merging activity.
