The galaxy presents as a moderately bright, elliptical-like structure. Its central region exhibits a pronounced yellow-orange hue, suggesting a population of older stars. The galaxy lacks distinct spiral arms. The overall color profile suggests a relatively quiescent star formation rate. The morphology appears generally smooth with no obvious major disturbances, although a slight asymmetry could suggest a minor tidal interaction. The estimated size is roughly 3.6 kpc. The galaxy exhibits a notable presence across the g, r, and z bands, indicating a substantial stellar population.
