The galaxy presents as a relatively smooth, elliptical object with a discernible core. The core exhibits a reddish hue, possibly indicative of an older stellar population. The main body of the galaxy is elongated, appearing cigar-shaped with one end slightly more disturbed. There is a hint of a disk-like structure around the central bulge, though it is not sharply defined. A blue tint across the galaxy suggests the presence of some younger, hotter stars or a small amount of star formation, though overall the galaxy appears to be relatively quiescent in terms of star formation activity. No obvious spiral arms or major merger events are evident, but there might be minor tidal disturbances. The overall morphology suggests a galaxy transitioning toward a more passive, spheroidal state.
