The galaxy presents as a somewhat elongated, spindle-shaped structure. The central region exhibits a brighter, more concentrated luminosity, suggesting a denser stellar population or possibly an active galactic nucleus. The color gradient transitions from a warmer, slightly reddish hue in the central bulge to a cooler, bluer color towards the outer edges. The overall morphology appears relatively smooth, with no immediately discernible spiral arms or prominent dust lanes. The galaxy shows no obvious signs of major interaction or merging events, though there is a hint of a slight asymmetry in the outer halo, suggesting a possible minor tidal disturbance or recent accretion event. The galaxy is relatively large, in terms of physical size, appearing as an elliptical galaxy in form. The star formation rate seems to be low in this galaxy.
