The galaxy presents an elliptical morphology, with a smooth, featureless appearance and a lack of discernible spiral arms or a central bar. The galaxy's shape is somewhat elongated, exhibiting a moderate ellipticity; it appears more in-between round and cigar shaped. The color profile suggests a population dominated by older stars, exhibiting a redder hue, likely due to the diminished presence of young, blue stars associated with active star formation. There are no evident signs of ongoing mergers or major tidal disturbances in the surrounding area, nor strong evidence of significant star formation, with the galaxy appearing largely quiescent. Overall, this appears to be a relatively isolated, evolved galaxy.
