The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The light distribution suggests a dominant bulge component, indicated by the concentration of yellow-orange light towards the core. Fainter blue light is present in the outskirts, possibly indicative of some ongoing, low-level star formation, though the overall color suggests a population dominated by older stars. There is no obvious spiral structure or distinct features such as tidal tails or strong asymmetries, suggesting it is likely a relaxed system without recent major merger activity. There may be subtle disturbances or faint arms, but the resolution of the image limits detailed morphological classification. The color gradient from the central bulge to the outer regions is gradual, which is consistent with the transition between the older stellar population in the bulge and the younger stars in the disk. The galaxy's relatively compact appearance and lack of strong star-forming regions point toward it being a fairly evolved system.
