The galaxy appears as a singular, moderately sized object, exhibiting a smooth morphology with a predominantly round shape. There's an indication of a slight radial concentration of light towards the center, suggesting a possible bulge component. The galaxy's color profile indicates it is more red than blue, suggesting a stellar population that is relatively old. There is no discernible disk or spiral structure. There are no visible signs of ongoing major merger activity or significant tidal disturbances. The galaxy does not appear to be interacting with any other object within the immediate vicinity.
