The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, appearing mostly rounded rather than elongated. The color profile suggests a dominant population of older stars, indicated by the redder hue in the galaxy's central region. There's minimal evidence of spiral arm structure or significant dust lanes; it appears largely featureless at this resolution. The luminosity profile indicates a lack of intense star formation. The galaxy does not appear to be undergoing any major merging events, though some minor asymmetry or a slight distortion could suggest a past interaction. Its relatively compact size implies a moderate physical scale.
