The galaxy presents as a smooth, elliptical morphology. Its light profile appears relatively uniform, with a central concentration that gradually fades towards the edges. The color indices suggest a redder population of stars, likely indicative of an older stellar population with ongoing but relatively low levels of star formation. The galaxy's shape is elongated, exhibiting a cigar-like appearance. There's no strong evidence of spiral arm structure or significant dust lanes. Based on the morphology, the object appears to be a relatively undisturbed galaxy, showing little sign of recent major mergers or tidal interactions.
