The galaxy presents as a slightly elongated, lenticular structure. Its overall color profile is indicative of an older stellar population, appearing predominantly yellowish, concentrated in the central bulge region. There is a subtle gradation towards redder hues in a ring around the bulge, perhaps indicating areas of older stars and dust absorption. The galaxy's structure is fairly smooth, lacking any distinct spiral arms or significant irregular features that would point towards recent major merger activity. It exhibits moderate rotational symmetry. The small disturbances observed suggest that it is likely either an elliptical galaxy or an early-type spiral galaxy with a tightly wound disk. The galaxy is relatively compact in appearance, lacking any extended halo or tidal debris. The star formation is estimated to be low.
