This galaxy exhibits a generally smooth morphology. The light distribution suggests a centrally concentrated spheroid shape with a moderate ellipticity, appearing somewhat elongated. It displays a yellow-white hue in its central region, likely indicating an older stellar population dominating the core. Fainter, bluer emission extends outwards from the central region, possibly indicating ongoing star formation. There is no readily apparent spiral arm structure or bar feature visible. The overall impression is of a galaxy transitioning between a spiral and elliptical form, with a mix of old and potentially young stellar populations. There are no significant tidal disturbances or signs of an ongoing major merger event visible.
