The galaxy presents a predominantly smooth morphology, exhibiting a high degree of radial symmetry. Its shape appears largely round. There is no obvious spiral arm structure or significant dust lane features. The light distribution is concentrated towards the center, suggesting the presence of a substantial bulge component. Perturbations or tidal features indicative of recent major merger activity are largely absent, although there may be a very slight disturbance visible. The galaxy has a redder color, suggesting an older stellar population and potentially a lower rate of ongoing star formation. The overall luminosity is relatively high, indicating that it is a massive galaxy.
