The galaxy appears to be a relatively small, elliptical galaxy at a redshift of approximately 0.055. The galaxy's morphology is smooth, and it has a somewhat elongated, cigar-like shape. There is no indication of significant disk structure, or any major ongoing merger activity. The blue hue suggests some recent or ongoing star formation, though the overall star formation rate appears low. The galaxy's color is brighter in the center and fades as it gets farther out from the center. There are no obvious spiral arms or dust lanes visible. The system is likely a relatively old galaxy, with a stellar mass in the range of 10^8 solar masses. There are no indications of tidal tails or other disturbances, suggesting that the galaxy is relatively isolated or has settled after a past interaction.
