The galaxy appears as a relatively smooth, centrally concentrated object with a slight elongation. It exhibits a color gradient, transitioning from a more yellowish hue at the core to a redder outer region. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy appears undisturbed, with no obvious signs of ongoing mergers or tidal interactions. The smoothness suggests an older stellar population and reduced star formation activity. The effective radius appears to be around 3 kiloparsecs.
