The galaxy appears to be a relatively compact and luminous object. It presents with a generally smooth morphology, exhibiting a slight elongation but no obvious spiral arm structures or prominent disk features. The central region shows a higher surface brightness, suggesting a concentrated nucleus. Faint diffuse emission extends outwards from the core, fading into the background sky. There is a subtle hint of minor disturbances or tidal features, though they are not prominent. Overall, the galaxy exhibits a morphology consistent with an elliptical or lenticular type, with indications of low star formation activity. The color indices suggest that it is composed of an older stellar population.
