The galaxy presents as a single, largely homogenous object with a centrally concentrated light profile. The overall morphology appears elliptical with a smooth, diffuse glow, indicative of an early-type galaxy. A slight elongation is perceptible, deviating marginally from a perfectly circular shape. The color is yellowish-orange, which suggests a population of older stars and a lower rate of on-going star formation. No distinct spiral arms, dust lanes, or active star-forming regions are discernible. There might be a slight hint of a stellar halo extending beyond the main body of the galaxy, but this is not well-defined. There are no signs of any current major merger events or significant tidal disturbances. It appears to be a relatively undisturbed, evolved system.
