The galaxy presents an elliptical morphology, appearing somewhat elongated with a cigar-like shape. The light profile seems relatively smooth with no apparent spiral arm structures or significant dust lanes visible in this image. A prominent central bulge is observed, exhibiting a concentration of light and a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear more diffuse and bluer in color, potentially indicating the presence of some younger stars or ongoing, though limited, star formation. There is a hint of some minor disturbance in the overall structure, potentially indicative of a past or ongoing interaction. The galaxy does not appear to be undergoing a major merger, however.
