The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. It has a generally rounded shape but appears slightly elongated, somewhere between round and cigar-shaped, indicating a possible oblate spheroidal structure. A concentration of light emanates from the galactic center, gradually decreasing in intensity towards the outer regions. There is some indication of color variation, with a yellowish hue near the center potentially indicating an older stellar population, while some regions exhibit a slight bluish tint that could be indicative of more recent, but limited, star formation, possibly around 10^2 solar masses per year. There is no obvious spiral arm structure or a prominent disk. The surrounding field shows no major signs of tidal distortion or interaction with other galaxies, indicating the galaxy is relatively isolated and has not experienced a recent major merger. Minor disturbances cannot be ruled out completely. The overall appearance is consistent with an early-type galaxy that is still undergoing minor star formation.
