The galaxy presents as a slightly elongated, cigar-shaped object. It exhibits a smooth, though not perfectly uniform, light distribution. The central region appears brighter and more concentrated than the edges. The color profile suggests a mix of stellar populations, with a subtle blue hue along the periphery indicating regions of potentially ongoing star formation and redder tones in the core likely indicating older stars. There is no apparent spiral structure or significant dust lane visible in the image. The general morphology suggests the galaxy is an elliptical or lenticular type, exhibiting minimal disturbances or merging activity.
