The galaxy presents as a relatively compact object, approximately 6 kiloparsecs in radius, with a moderate redshift indicating significant distance. The central region exhibits a smooth morphology, appearing largely spheroidal in shape. Light distribution is concentrated towards the core. The color profile suggests a population of older stars within this spheroid.

There are no strong indications of ongoing major mergers. It shows signs of potential tidal tail. Star formation rate appears subdued, as indicated by the muted blue tones observed. Overall, this galaxy displays characteristics consistent with an evolved system where star formation activity has decreased over time.
