The galaxy presents as a generally smooth, elliptical structure with an apparent cigar shape. The central region exhibits a concentrated, bright yellowish-white luminosity, suggestive of an older stellar population. The isophotes become less defined and redder towards the outer regions of the galaxy, likely due to a decreasing stellar density and possible presence of dust. There's no discernible evidence of spiral arms or a distinct disk component, nor is there any indication of any major ongoing merging activity, though minor disturbances cannot be ruled out. The galaxy's apparent red color indicates that star formation is limited or has largely ceased, giving it an older stellar population. The overall morphology points towards an evolved system.
