The galaxy presents as a centrally concentrated system, exhibiting an elliptical morphology. The light distribution appears smooth with an even gradient. The galaxy appears elongated, exhibiting a cigar-like appearance, but a fair amount of light is also distributed in a more rounded region closer to the center. I do not detect any strong spiral arm features or bar structures. The color profile indicates a dominant population of older stars and lower levels of on-going star formation. There is evidence of slight disk component. No signs of major mergers or strong tidal disturbances. The galaxy appears relatively isolated, with no immediate companion galaxies visibly interacting. Overall, the galaxy appears as a somewhat early-type system nearing completion of its star formation.
