The galaxy appears to be a relatively smooth, elliptical system. Its morphology is dominated by a centrally concentrated bulge, exhibiting a radial gradient in luminosity, with the core being significantly brighter. The light distribution suggests a high degree of spherical symmetry, with only minor deviations from a perfectly circular shape. There is no obvious indication of spiral arms, a bar structure, or significant dust lanes. The galaxy appears to be relatively isolated, showing no signs of ongoing major mergers or tidal interactions. It exhibits a blue hue suggesting active star formation.
