The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular, with a slight deviation from perfect roundness. The core of the galaxy exhibits a high surface brightness, indicative of a concentrated stellar population. Diffuse light extends outward from the central region, diminishing gradually towards the edges. There is little to no discernible structure within the disk, and there is no readily apparent spiral arm structure. No major mergers or tidal disturbances are observed. The color profile suggests a galaxy dominated by older stellar populations, with a relatively small rate of ongoing star formation.
