The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall morphology suggests an elliptical or lenticular classification. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population, while the outer regions display a gradual decline in surface brightness, transitioning to a more reddish color. There is no clear evidence of prominent spiral arms or significant dust lanes, implying a limited ongoing star formation rate. The galaxy appears to have a moderately high mass with a redshift of roughly 0.15. There are hints of a slight deviation from perfect roundness; however, the overall structure seems largely undisturbed, with no obvious signs of recent major merger activity or tidal features.
