The galaxy presents as a smooth, elongated structure, closely resembling a cigar shape. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The central region exhibits a slightly brighter concentration of light. The color gradient transitions subtly from a slightly redder hue towards the center to a bluer tint at the outer edges, possibly indicating a difference in stellar populations and activity. There appear to be no major disturbances or interactions with other galaxies. Overall, the morphology suggests a galaxy dominated by an older stellar population with low star formation activity.
