The galaxy presents a generally smooth morphology, with no obvious spiral arm structures or bar. The central bulge region appears to be a dominant feature, exhibiting a high degree of luminosity and a nearly spherical shape. The galaxy's light profile appears centrally concentrated, with the intensity diminishing gradually from the core outwards. There is little evidence of significant dust lanes or patches. The overall color index suggests a population dominated by older stars, contributing to its yellowish-orange hue. The galaxy's outskirts seem diffuse, without a sharply defined edge, potentially indicative of an extended halo.
