The galaxy presents as a somewhat elongated, moderately bright object with a smooth overall appearance. It exhibits a reddish hue, which may indicate an older stellar population or significant dust obscuration. The morphology appears to be somewhere between round and cigar-shaped, not showing a distinct disk. There does not appear to be significant evidence of tidal disturbances or a major merger event in progress, though a faint asymmetry cannot be ruled out. Based on the color profile, the galaxy is likely an elliptical galaxy at an approximate distance of roughly 0.26 in redshift, likely a population of older stars that are no longer forming.
