The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology. The galaxy is roughly elliptical in shape, with a brighter, concentrated central region that fades into a more diffuse halo. There is some evidence of a faint disk-like structure, but it is not well defined. The color profile suggests an aging stellar population, with a dominance of redder hues particularly within the central bulge. The overall structure does not show any obvious signs of ongoing major mergers or significant tidal disturbances, but there may be minor irregularities suggesting possible past interactions. Star formation activity is likely low, consistent with the lack of strong blue colors typically associated with young, hot stars.
