The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology with no obvious spiral arm structure or significant dust lanes visible. The galaxy core appears bright and moderately compact, suggesting a possible active galactic nucleus or a dense concentration of stars in the nuclear region. The color profile indicates a population of older stars, trending toward redder hues, especially in the outer regions. There is minimal evidence of on-going star formation. Overall, the galaxy appears to be a mature system with a low rate of star formation and no significant merger activity.