The galaxy presents as a centrally concentrated elliptical or lenticular morphology. It appears largely smooth with no immediately apparent spiral arm structure. The galaxy exhibits a pronounced central bulge that gradually fades into a more diffuse halo. The core is bright, suggesting a high concentration of stars. The color profile indicates a primarily older stellar population, exhibiting a yellow-red hue, with little evidence of ongoing active star formation within the main body. There's no sign of active galactic nucleus. The galaxy seems to be isolated, without significant tidal distortions or interactions with other nearby galaxies, although a very subtle disturbance is possible in the outer regions.
