The galaxy presents as a single, moderately luminous object with a centrally concentrated brightness profile, suggesting an elliptical morphology. The light distribution appears relatively smooth with no obvious spiral arm structures or prominent dust lanes. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. Surrounding the core, a bluer component is observed, potentially caused by a younger stellar population compared to the core. There is no morphological evidence of recent major mergers. Minor disturbances are possible, but not definitively observed from this image. The overall shape is somewhat rounded, verging on elliptical.
