This galaxy exhibits a generally smooth morphology, with a concentrated central bulge and a diffuse halo. Its overall shape appears somewhat elliptical, but with a slight deviation from perfect roundness. The color gradient suggests a higher concentration of older stellar populations in the central region, indicated by the yellow-orange hue, transitioning to bluer colors in the outer regions, potentially signifying more recent star formation. There is little evidence of prominent spiral arms or a well-defined disk structure. Some subtle irregularities or minor disturbances can be observed within the galaxy's extended halo, though no major signs of ongoing mergers or strong tidal interactions are apparent. The galaxy appears relatively isolated, lacking any immediately interacting companion galaxies in the observed field.
