The galaxy presents as a relatively bright, isolated object. Its overall morphology appears elliptical, with a smooth, concentrated light distribution, lacking prominent spiral arms or distinct features. There is a slight elongation, suggesting it is not perfectly spherical. Its core appears the brightest. The color profile suggests that the galaxy has some older stars. The lack of obvious dust lanes or knots of star formation reinforces the impression of a galaxy dominated by an older stellar population, indicative of relatively low ongoing star formation activity. There appears to be no significant interaction or merging events. There appears to be very minor asymmetry.
