The galaxy presents as a slightly elliptical, moderately luminous system. Its central region appears bright and concentrated, exhibiting a yellowish-orange hue, suggesting an older stellar population. The outer regions display a fainter, diffuse structure with hints of bluer colors, possibly indicating the presence of some younger stars, though these are not prominent. There is no obvious spiral structure or bar visible. There appears to be some slight asymmetry to the galaxy, potentially suggestive of past or ongoing interactions, though no strong tidal features or major distortions are apparent. The overall morphology seems to be somewhere between a disk galaxy and an elliptical, perhaps a lenticular type.
