The galaxy presents a generally smooth morphology, exhibiting a largely featureless appearance in this image. It shows a centrally concentrated light profile, appearing quite round with only minor deviations from perfect circularity. The galaxy's color suggests a relatively evolved stellar population, exhibiting a redder hue. No pronounced spiral arms, bar structures, or dust lanes are discernible, further supporting its classification as a likely elliptical or lenticular galaxy. There is no obvious evidence of any major ongoing mergers or significant tidal disturbances in the immediate vicinity of the galaxy. The light from the object is likely dominated by older stars rather than newly forming populations.
