The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular classification. The light is concentrated towards the center. It appears moderately elliptical in shape, with the ratio of the major to minor axes being roughly estimated at 2:1. No distinct spiral arm structures or prominent dust lanes are discernible. The color is predominantly blue, hinting at a population of younger, hotter stars and indicating ongoing or recent star formation, though the overall rate appears relatively low. There is a faint hint of a possible disturbance or tidal feature. This requires deeper imaging for confirmation. The size is rather modest, with the half-light radius estimated to be approximately 1.4 kpc. 
