The galaxy appears to be a relatively smooth and elliptical structure with a concentrated central bulge. It exhibits a yellowish-orange hue, suggesting an older stellar population with a lower rate of ongoing star formation. There is little to no discernible spiral arm structure or prominent dust lanes. The overall morphology is consistent with an early-type galaxy, specifically a spheroidal galaxy. There is no evidence of tidal disturbances or other signs of recent merger activity.
