The galaxy presents as a smooth, elongated object with a cigar-like shape. The light distribution suggests a central bulge dominating the structure, with a noticeable color gradient, trending from a slightly bluer core towards redder, more diffuse outer regions. There is no visible spiral structure or distinct disk component. The smooth profile and color distribution could indicate a relatively evolved system with a lower rate of ongoing star formation compared to galaxies with prominent spiral arms or irregular features. There is no evidence of any major mergers or tidal disturbances. Overall, the galaxy appears to be an elliptical or lenticular type, viewed at a considerable angle relative to its plane.
