The galaxy presents a largely smooth morphology, exhibiting characteristics of an early-type system. It appears elliptical in shape, though not perfectly circular, possessing a slight elongation along a discernible axis. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions.  

The color profile suggests a relatively passive stellar population, displaying a redder hue.  There is no apparent spiral structure or significant dust lane obscuration evident in the available imagery.  Faint indications of a minor asymmetry or tidal feature is noted in the lower left. The overall impression is that of a mature galaxy with a spheroidal component dominating its structure.
