The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. It displays a subtle elongation, deviating from a perfectly circular shape. The galaxy's color profile suggests a predominantly older stellar population, with a yellowish hue indicating a lack of significant recent star formation. No distinct spiral arms or dust lanes are visible, further supporting its classification as an elliptical galaxy. There is no evidence of any major merger events. The galaxy seems to be relatively isolated, with no apparent tidal interactions with neighboring galaxies.