The galaxy presents as a single, concentrated body with a smooth, mostly spheroidal morphology. It displays a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of recent star formation. There is no apparent spiral structure or distinct disk. The light profile appears centrally concentrated with a gradual fall off in intensity further from the center, and has a roughly round shape, with a slight deviation. There is no indication of any recent major merging events or significant tidal disturbances. There might be minor disturbances within the galaxy but further analysis would be needed to determine if these are artefacts or signs of a minor merging event.
