The galaxy presents a relatively smooth, elliptical morphology. Its light profile appears centrally concentrated with a gradual decline in brightness outward from the core. There is a hint of faint, diffuse structure extending from the main body of the galaxy, but no distinct spiral arms or bar features are readily apparent. The color suggests a population of older stars, with a general absence of bright blue star-forming regions. The galaxy exhibits an overall yellowish-red hue indicating that its recent star formation rate is very low. The object's shape is generally rounded. While appearing relatively isolated, there may be some minor tidal disturbances, but the presence of a major merger is unlikely.
