The galaxy presents as a somewhat smooth, elliptical-like structure, though not perfectly rounded. It appears slightly elongated. A central bulge region is visible, exhibiting a concentrated, bright yellowish-orange hue, suggesting a population of older stars. Surrounding the bulge, a fainter, more diffuse disk or halo is observed, displaying a bluish tinge in certain areas. This bluer color might indicate regions of ongoing star formation. There is no clear evidence of strong spiral arm structures or major disturbances due to interactions or mergers, although a slight asymmetry or minor perturbation cannot be entirely ruled out. The galaxy seems to be relatively isolated, showing no signs of close companions or tidal tails. Based on the observed color gradients, the galaxy likely contains a mixture of stellar populations, with older stars dominating the central regions and younger stars contributing to the outer regions. Overall, the galaxy appears to be relatively evolved, with potentially moderate levels of recent star formation.
