This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile with a largely spheroidal shape. The galaxy's core is characterized by a yellowish-white hue, possibly indicative of an older stellar population dominating the central region. Moving outward from the core, the color transitions to a bluer gradient, suggesting the presence of some younger, bluer stars at the outskirts, although these do not appear prominent. No distinct spiral arms or other large-scale structures such as bars are readily apparent. Overall the galaxy does not seem to be undergoing any major merger activity, although there appears to be slight asymmetries. The angular size suggests a relatively compact system with a moderate amount of overall luminosity. The redshift implies that the light from this galaxy has been traveling for a considerable amount of time, so the overall view is potentially of the galaxy in its past.
