The galaxy presents as a centrally concentrated object with a smooth light distribution. Its overall morphology appears elliptical, exhibiting a notable degree of roundness with a slight tendency towards an elongated shape. The central region displays higher brightness, gradually fading towards the outer edges. There's a subtle bluish hue in the central and inner regions of the galaxy, potentially indicative of ongoing star formation or a population of relatively young stars. Overall, there is no obvious signs of major disturbances or mergers, though there may be minor irregularities in the light distribution. Its redshift indicates it is a relatively distant object. The galaxy appears to be a regular elliptical galaxy with no significant morphological peculiarities.
