The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears elliptical or spheroidal. The light distribution suggests minimal evidence of spiral arms or a prominent disk structure. The color gradient observed shows a centrally located, bright core region with a yellowish hue. Surrounding this core, a less intense, greenish halo is visible, extending outwards. There is a subtle indication of possible minor disturbances or interactions, but no definitive signs of major mergers or tidal features can be seen in the available imagery. The estimated size of the galaxy is around 4.4 kpc. Despite its relatively smooth appearance, the presence of the extended greenish halo could signify ongoing or recent star formation activity, however, star formation appears subdued overall.
