The galaxy presents as a somewhat elongated, diffuse object, likely an elliptical galaxy given the lack of discernable spiral arms or a prominent disk structure. The central region exhibits a higher surface brightness, suggesting a concentrated stellar population or a possible active galactic nucleus, though the resolution is insufficient to confirm the latter. The galaxy displays a smooth, featureless appearance, with no apparent dust lanes, tidal tails, or other signs of recent mergers or interactions. The color appears relatively uniform across the galaxy, with a slight tendency toward redder hues, which is consistent with an older stellar population and low star formation rate. The observed shape deviates from a perfect circular form, indicating a degree of ellipticity. There is no evidence of significant ongoing star formation within the galaxy, suggesting that it is a relatively passive system.
