The galaxy presents as a somewhat smooth, elliptical-like object, with a notable central bulge that appears to be a dominant feature. The core exhibits a yellowish-white hue, which may indicate an older stellar population, with relatively low rates of current star formation. The gradient of color indicates a more substantial population of older stars in this region. The overall shape appears elongated rather than perfectly spherical. Some slight distortions in the outer regions are potentially visible, suggesting past or ongoing gravitational interactions. The galaxy does not show prominent spiral arm structures. The diffuse nature of the galaxy suggests a lack of significant dust lanes or regions of active star formation.
