The galaxy presents as a moderately bright, elliptical structure. The light is concentrated towards the center of the galaxy, exhibiting a smooth, almost featureless profile. The overall shape appears somewhat rounded, though verging on elliptical with no obvious disc structure discernible at this resolution. There are no strong indications of spiral arms or prominent dust lanes. The color profile suggests a population of older stars, leaning towards yellow and redder hues. There are no evident signs of ongoing major merger activity or significant tidal distortions in its morphology, although some minor asymmetries cannot be entirely ruled out.
