The galaxy presents as a centrally concentrated, relatively smooth object with a moderate redshift. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Surrounding this core is a more diffuse, fainter halo, tinged with blue. This may indicate the presence of some younger stars, although their overall contribution to the galaxy's light is minor compared to the core. The galaxy's overall shape is moderately elliptical. No distinct spiral arms or significant dust lanes are discernible, and there is no evidence of ongoing major mergers or tidal disturbances. The overall morphology suggests a galaxy in the process of settling into a more quiescent state, with a relatively low star formation rate.
