The galaxy presents an elongated, cigar-shaped morphology, indicative of an elliptical or lenticular classification. The light distribution appears relatively smooth, with a concentration towards the center, suggesting an older stellar population. A subtle color gradient is observed, with a redder hue in the core gradually transitioning to a slightly bluer tinge in the outer regions, possibly indicating recent star formation in the galaxy's disk. There are no apparent strong tidal features or distortions, suggesting a relatively isolated evolutionary history.
