The galaxy presents as a relatively compact object with a moderately smooth morphology. It appears to be somewhat elliptical in shape, displaying a slight elongation. There is a subtle color gradient visible, with a tendency toward redder hues in the central regions, potentially indicative of an older stellar population or dust obscuration. Fainter, bluer regions are observed in the outer parts of the disk, hinting at possible ongoing star formation activity. Visual inspection suggests the galaxy is likely not undergoing a major merger, though minor disturbances or tidal features cannot be completely ruled out given the image resolution. Overall, the galaxy exhibits characteristics consistent with a transitioning type of galaxy, possibly between a spiral and an elliptical, with evidence of diminished star formation.
