The galaxy presents an overall smooth and centralized morphology, suggesting a relatively evolved system. A bulge component is evident, appearing concentrated and exhibiting a yellowish hue, indicative of an older stellar population. The disk is discernable but less prominent, displaying a fainter, bluish tint, suggestive of ongoing, albeit moderate, star formation activity. There is a slight asymmetry to the outer regions of the disk, potentially indicative of a minor gravitational disturbance or past interaction. The galaxy's overall shape is somewhere in between round and elongated. No strong signs of major merger events or significant tidal features are immediately apparent. The galaxy appears relatively isolated within the observed field.
