This galaxy presents a primarily smooth, elliptical morphology. There is a slightly elongated shape, suggesting a possible classification between an elliptical and a lenticular galaxy. The central region exhibits a concentrated, bright yellowish glow, indicating a significant population of older stars. A subtle, diffuse bluish hue surrounds the core, which could be evidence of younger star formation, though appearing subdued. There is no significant sign of spiral arms. There's also no apparent presence of a major merger, though the asymmetry could suggest a past minor disturbance or ongoing interaction. The galaxy appears relatively isolated.
