The galaxy presents a generally smooth and rounded morphology, appearing largely featureless. The light distribution is concentrated towards the center, indicating a prominent bulge. The central region exhibits a yellowish-orange hue, which could suggest an older stellar population. Moving outwards from the center, the color transitions to a slightly bluer tint, which could indicate a presence of younger, hotter stars. The absence of distinct spiral arms or a bar structure suggests a classification towards early-type galaxies. There is no visual evidence of any major mergers or tidal disturbances, which may indicate that the galaxy is relatively undisturbed and isolated.
