The galaxy presents a somewhat elliptical morphology, appearing more elongated than circular. The overall color profile suggests a population of older stars, with a reddish-yellow hue dominating the core and extending outwards. A lack of defined spiral arm structure or distinct features suggests a relatively smooth stellar distribution. There may be very minor dust lanes visible upon closer inspection, but overall the galaxy appears to be well evolved. The central bulge appears prominent, and a faint disk component could be present based on the overall shape of the light distribution. There does not appear to be any active star formation.
