The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of central concentration. The object appears largely featureless with a round shape and no obvious spiral arm structure or significant tidal disturbances are visible in the image.  The color profile suggests a population of older stars, with a relatively weak signature of active star formation. This is based on the redder overall color. There is no evidence of a major ongoing merger or significant interaction with a neighboring galaxy.
