The galaxy presents as a slightly elongated, lenticular structure with a smooth, diffuse light profile. There is a subtle central bulge that is brighter compared to the outer regions, gradually fading into the surrounding background. The overall color of the galaxy appears to be bluish-white, indicative of a moderate presence of younger, hotter stars, however its rate of star formation is likely low. The galaxy does not display any prominent spiral arms or significant dust lanes within the observable resolution. The shape is generally somewhere between a perfect circle and elongated cigar. There is evidence of a minor gravitational disturbance or interaction, which suggests that the galaxy has likely merged with, or is merging with a smaller galaxy.