The galaxy presents a largely smooth morphology, exhibiting minimal discernible features such as spiral arms or a prominent disk. The galaxy's light profile appears relatively uniform and concentrated, suggesting a spheroid-dominated structure. There is a slight color gradient, trending towards redder hues in the central regions and slightly bluer tones in the outskirts.

The overall shape appears approximately round, with a subtle elongation that is more in between round and cigar shaped. There are no obvious signs of ongoing major merger activity or significant tidal disturbances, though some minor asymmetry might indicate past interactions or internal dynamics. The galaxy's size appears moderately extended relative to other field objects, likely corresponding to a significant physical diameter. Overall star formation rate is low, which aligns with the smooth morphology and redder colors.
