The galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The color profile suggests a population of older stars, indicated by the reddish-orange hue dominant in the central bulge. There is little evidence of well-defined spiral arm structure or significant dust lanes. The galaxy appears to be generally spheroidal in shape, with a slight elongation. A faint disk component is potentially present, though not readily apparent. Signs of tidal disturbances or ongoing mergers are not immediately obvious.