The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape, appearing mostly round with a slight elongation. The light profile suggests a relatively featureless structure, indicative of a galaxy dominated by an older stellar population. There is a hint of a faint extended halo or envelope surrounding the central luminous region. Coloration is subtle, with a slightly bluer hue in the center, transitioning to redder tones in the outer regions, which may suggest ongoing or recent star formation, especially in its core. There is no prominent presence of spiral arms or significant dust lanes, further supporting the classification as a probable elliptical galaxy. There are no obvious signs of tidal interactions or ongoing mergers, suggesting a relatively isolated system.
