The galaxy appears as a centrally concentrated, smooth object with a generally elliptical morphology. Its core exhibits a bright, yellowish hue, suggesting a population of older stars. The light gradually fades towards the outer regions of the galaxy. There are faint hints of a more extended, diffuse halo surrounding the central region, though distinct spiral arm structures or prominent dust lanes are not discernible from the image. The overall visual impression is that of a relatively undisturbed system, with no strong evidence of ongoing major merger activity.
