The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with the ratio of minor to major axes indicating a moderate ellipticity. The galaxy's color profile suggests a population of older stars dominating its stellar content, potentially indicating a relatively passive star formation history. No prominent spiral arm structures or significant dust lanes are visible. Faint irregularities in the light distribution may be indicative of minor past or ongoing interactions, but a generally undisturbed morphology is observed. The apparent size suggests it is a relatively compact galaxy at its redshift, and its luminosity points to a considerable mass.
