The galaxy appears as a centrally concentrated object with an elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a significant population of older stars. Moving outward from the core, the galaxy gradually transitions to a fainter, more diffuse halo with a slightly redder tone. There is no apparent spiral structure or distinct disk component visible in this observation. The galaxy appears relatively smooth in texture, without any obvious signs of recent major mergers or significant tidal disturbances. Overall, the galaxy appears to be a fairly relaxed system, likely dominated by an older stellar population, with a low rate of ongoing star formation.