The galaxy presents as an elongated, somewhat cigar-shaped object. It exhibits a smooth, centrally concentrated light distribution, suggesting a lack of prominent spiral arm structures. The core region shows a yellowish hue, potentially indicating an older stellar population. The outer regions appear bluer, possibly reflecting ongoing, albeit limited, star formation activity. There is no clear evidence of tidal features or major disturbances to the overall morphology, suggesting it is not currently undergoing a major merger. The galaxy seems relatively isolated and undisturbed.
