The galaxy exhibits a somewhat lenticular morphology, appearing as a flattened spheroid. The light distribution is concentrated towards the center, suggesting a prominent bulge component. The overall color is yellowish-orange, indicating a population of older stars with less ongoing star formation. There is a slight asymmetry in the light distribution and an indication of minor disturbances within the galaxy. The central region is smooth and lacks significant dust lanes or spiral arm features, suggesting a relatively quiescent galaxy. Based on the observed color and morphology, this galaxy likely consists primarily of evolved stars with a minimal amount of gas and dust.
