The galaxy appears to be a relatively smooth, elliptical type galaxy. Its light profile is centrally concentrated, fading gradually outwards with no distinct spiral arm structures. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population, with less dust and gas obscuration. There is a slight blue tint towards the outer regions of the galaxy, potentially indicating the presence of some younger, hotter stars, albeit in relatively small quantities. The overall roundness and lack of significant distortions suggest that the galaxy is relatively undisturbed. There's no clear evidence of ongoing major mergers or tidal interactions. The colors indicate ongoing, but relatively low, star formation. Overall, it seems to be a somewhat massive galaxy with moderate ongoing star formation, likely dominated by evolved stars and with little dust obscuration.
