The galaxy presents as an elongated, cigar-shaped system. A smooth, diffuse central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The galaxy's disk component appears relatively smooth and somewhat featureless, lacking prominent spiral arm structures. There is a hint of blueish color within the disk, possibly indicative of ongoing star formation, albeit at a low rate. A smaller, brighter object is located near the galaxy and appears to be undergoing a merger or tidal interaction. There is no evidence of a strong central active galactic nucleus. Overall, the galaxy appears to be a relatively evolved system with a moderate mass and a low specific star formation rate.
