The galaxy presents as a centrally concentrated object, elongated in shape, with a noticeable color gradient. The core appears to be a reddish-orange hue, suggesting an older stellar population. The outer regions exhibit a slight greenish tinge. The galaxy has a smooth appearance without any obvious spiral arm structures or prominent dust lanes. The elliptical morphology and color profile indicate that this is likely an evolved galaxy with ongoing, but perhaps diminished, star formation. There are no clear indications of a major merger, although subtle irregularities might suggest minor disturbances or past interactions. The galaxy's overall structure appears relatively stable.