The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a high degree of central concentration. The light distribution is not perfectly uniform, and shows that it is more in between disk shaped and round. A slight elongation is observable, suggesting a possible cigar shape, however not to a high degree. Color gradients within the galaxy reveal a predominantly yellow-orange hue in the central region, indicative of an older stellar population. The outer regions display a subtle bluer tint, possibly signifying the presence of younger, hotter stars, and perhaps some ongoing, but subdued, star formation. Evident disturbance present, possibly from a recent minor merger or tidal interaction.
