The galaxy exhibits a generally elliptical morphology, appearing largely smooth and spheroidal. The central region displays a concentrated luminosity gradient, indicative of a prominent galactic nucleus. The galaxy's color profile seems to lean towards the redder end of the spectrum, suggesting a population of older stars. There is little evidence of significant dust lanes or spiral arm structures; the overall form is relatively homogenous. The outer regions display a gradual decrease in light intensity, fading smoothly into the background. There are very slight signs of disturbances in its morphology, but the galaxy appears largely undisturbed and relaxed.
