The galaxy presents a generally smooth and rounded morphology, appearing largely featureless at this resolution. The central region exhibits a concentrated luminosity, indicative of a prominent galactic bulge. A faint, diffuse halo surrounds the central region, exhibiting a subtle color gradient. This gradient transitions from a yellowish-white core to a slightly greenish-blue outer edge, suggesting possible variations in stellar populations or dust distribution. There is no readily apparent spiral arm structure or evidence of significant tidal disturbances. It appears to be relatively isolated, showing no clear signs of ongoing or recent major mergers.
