The galaxy appears as a centrally concentrated, relatively smooth object. There is a dominant, nearly spherical bulge. The color profile suggests a yellow-white hue in the central region, potentially indicative of an older stellar population. The outer regions exhibit a gradual color shift towards redder tones, which could reflect a change in stellar populations or dust content. There is a slight, nearly imperceptible disk structure. No spiral arms or distinct dust lanes are readily apparent, suggesting a more homogenous distribution of stars and interstellar material. There is no evidence of a recent major merger event or strong tidal distortions in the surrounding regions. Overall, the galaxy presents a moderately luminous, relatively quiescent morphology.
