The galaxy appears as a single, fairly symmetrical object. It exhibits a generally elliptical morphology, with no apparent spiral arm structures. Its light profile suggests a smooth distribution, with the majority of the luminosity concentrated in the central region, fading outwards. The color is generally a yellow-orange hue, possibly indicative of an older stellar population. There are no obvious signs of ongoing major mergers, although subtle disturbances cannot be entirely ruled out. It appears as if it is a very relaxed galaxy.
