The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core is bright, exhibiting a strong concentration of light. The overall color appears slightly redder, hinting at an older stellar population. The galaxy lacks any obvious spiral arm structures or prominent dust lanes. There is only a subtle color change going from the center of the galaxy to the outer parts. The overall shape suggests that the galaxy is not viewed face-on, but is presented with some degree of inclination. There is no evidence of ongoing mergers or major tidal disturbances. It appears to be a relatively isolated system, undisturbed by recent interactions.
