The galaxy appears to be a relatively compact object, generally elliptical in shape with a slightly irregular morphology. The core region exhibits a bright, concentrated luminosity, suggesting a higher density of stars or active galactic nucleus. There is evidence of ongoing or recent star formation, as indicated by the faint blue-ish color surrounding the central core, possibly indicating the presence of younger, hotter stars. The outer regions seem to fade into a redder hue, potentially implying an older stellar population. There are suggestions of minor disturbances or asymmetries in the galaxy's structure, possibly hinting at past interactions or minor merger events. The galaxy seems fairly isolated without evidence of significant tidal distortions, potentially implying a relatively quiescent evolutionary history.