The galaxy presents a relatively smooth morphology, with a noticeable disk-like structure but no clearly defined spiral arms. It displays a mostly elliptical form, appearing somewhat elongated. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. Overall, the galaxy appears to be actively forming stars at a moderate rate, as hinted by its blue light. There appears to be no signs of significant tidal disturbances or ongoing major mergers; however there is some minor disturbance. The color suggests a substantial population of older stars.
