The galaxy presents a largely smooth and rounded morphology. There is a noticeable concentration of light towards the center, suggesting a prominent galactic bulge. No distinct spiral arm structures or bar features are readily apparent. The galaxy appears relatively undisturbed, with no strong indications of ongoing major mergers or tidal disruptions. The color profile indicates a dominance of older stellar populations with a notable lack of blue stars, suggestive of a relatively low star formation rate. Overall, this galaxy appears to be a relaxed system dominated by evolved stars.
