The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The light distribution is dominated by a central bulge, fading gradually outwards. There is little evidence of spiral arm structure or significant dust lanes. The color gradient suggests a population of older stars. The galaxy is relatively isolated, showing no obvious signs of recent or ongoing major mergers, although subtle disturbances may be present. The overall structure indicates a relatively evolved system. There is some evidence of blue light, indicating some star formation.
