The galaxy presents a roughly elliptical morphology, appearing elongated in shape. The overall structure suggests a relatively smooth distribution of light, with no prominent spiral arms or distinct features immediately apparent. There appears to be a brighter concentration of luminosity towards the central region, which fades gradually towards the outer edges, implying a centrally condensed distribution of stars. The colors are generally subdued. There is a slight asymmetry, potentially indicating either a subtle interaction with another galaxy or some internal disturbance, though further data would be needed to confirm this hypothesis. Overall, this galaxy seems to be relatively undisturbed, with a smooth luminosity profile.
