The galaxy appears to be a spiral galaxy, viewed at a significant angle. The central bulge is prominent, displaying a yellowish-orange hue, which might indicate an older stellar population. There is evidence of a disk structure surrounding the bulge, marked by bluer regions that likely contain younger, hotter stars and ongoing star formation. The spiral arms are not clearly defined but are indicated by the subtle blue tinges extending outward from the bulge. There appears to be a companion object, to the side, that is red, and possibly related to the galaxy. The galaxy does not show strong signs of a major merger or significant tidal distortions, though there might be minor disturbances in its morphology. Overall, the galaxy seems relatively undisturbed, with an appreciable rate of star formation, and a substantial stellar mass.
