The galaxy presents a roughly elliptical morphology. It appears to be moderately inclined relative to our line of sight. The central bulge is prominent and bright, exhibiting a smooth, diffuse light distribution, suggesting an older stellar population. The outer regions display a fainter and more diffuse appearance, with a noticeable redder hue on one side, indicating potential dust lanes or regions of older stars. There is no obvious spiral arm structure visible. The overall structure suggests a relatively quiescent galaxy with little active star formation outside the central bulge region.
