The galaxy presents as an elongated, spindle-shaped structure. It appears to be relatively smooth in texture with a bright, concentrated core. The light gradually fades away from the center out towards the edges of the galaxy. The color profile suggests a population of older stars, indicated by the reddish hue towards the center, gradually shifting toward bluer tones towards the outer regions, which might indicate younger stars in the outer regions. There is a noticeable lack of defined spiral arm structures, lending further credence to a more elliptical morphology. Overall, the galaxy seems undisturbed, without significant signs of on-going mergers or tidal interactions.
