The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It has a subtle elongated shape, but generally lacks distinct spiral arm structures or a prominent bar. There is a suggestion of some minor disturbances in the light distribution, possibly indicating past or ongoing interactions with other galaxies. Its color suggests a population of older stars, with a relatively low rate of ongoing star formation. The object is reasonably massive and the morphology suggests it may be in the transition stage between a spiral and elliptical galaxy.
