The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The core exhibits a bright, yellowish-white hue, possibly indicative of an older stellar population. A gradual color gradient transitions outwards from the core to a more greenish-yellow tint, with hints of redder regions sporadically distributed along the galaxy's periphery. There is no evidence of distinct spiral arm structures or a prominent disk, suggesting a classification towards the elliptical or lenticular type. Faint, subtle disturbances or asymmetries are observed at the edges, potentially signifying minor interactions or ongoing merger events. Overall, the galaxy exhibits a generally undisturbed structure with a dominant, centrally concentrated luminosity profile.
