The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The primary body displays a predominantly yellowish-orange hue, suggesting a population of older stars. The smooth profile indicates a lack of significant spiral arm structure or prominent dust lanes. There is evidence of a smaller secondary object, likely a satellite galaxy, in close proximity to the primary galaxy. The satellite galaxy exhibits a similar color profile to the central galaxy. There is a noticeable color gradient, with the central core appearing brighter and slightly redder than the outer regions. This likely indicates an accumulation of older stars.
