This galaxy exhibits a morphology suggestive of an elliptical type. It presents with a generally smooth and concentrated light profile, with a high degree of central luminosity. There is a noticeable red-orange hue to the galaxy, hinting at an older stellar population with a diminished rate of star formation. The galaxy appears somewhat spheroidal in shape, and there seems to be a second galaxy nearby. There appears to be no clear evidence of strong tidal features or major disturbances, but further analysis would be needed to confirm its classification and interaction history with certainty.
