The galaxy presents as an elliptical or lenticular type, displaying a smooth, concentrated light profile. The central bulge appears dominant and exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse extensions of light are observed around the central region, contributing to a somewhat elongated morphology. There is evidence of possible gravitational interaction with a smaller, distinct bluish object nearby. The disk appears to be slightly disturbed. The galaxy does not present a strong visual indication of active star formation within the main body, though some is hinted at in the area of possible interaction.
