The galaxy presents as a relatively smooth, centrally concentrated object. It displays a somewhat elliptical morphology, with an apparent axis ratio suggesting a moderate inclination. The central bulge region exhibits a yellowish hue, likely indicative of an older stellar population and/or dust obscuration. Surrounding the central bulge is a fainter, bluer disk component. The galaxy is relatively isolated, showing no obvious signs of major tidal interactions or ongoing mergers, though there are some minor disturbances visible. It has an intermediate mass. The rate of star formation is low and the size is intermediate.
