The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with no obvious spiral arm structures or prominent dust lanes. The color profile suggests a dominant population of older stars, exhibiting a yellowish-orange hue at the core that fades to a more reddish color in the outer regions. There are subtle variations in color across the galaxy, which may indicate some level of ongoing or recent star formation, especially in its outer disk. The galaxy appears fairly isolated, with no obvious signs of tidal interaction or merging activity, the galaxy seems well-defined and undisturbed.
