The galaxy exhibits a generally smooth morphology, with minimal evidence of spiral arms or distinct features. The light distribution appears concentrated towards the center, suggestive of a prominent bulge. The galaxy displays a slightly elliptical shape, deviating marginally from a perfect circle. Color gradients are subtle, with a central region exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The outer regions show a slightly bluer tint, implying the presence of some younger stars, though star formation activity appears relatively low. No significant signs of tidal disturbances or ongoing mergers are readily apparent. The galaxy presents as a relatively isolated system.
