The galaxy presents a primarily smooth morphology, appearing as a single, consolidated object without readily discernible spiral arms or irregular features. It exhibits an elongated, cigar-like shape, suggesting an elliptical or lenticular classification. The central region displays a higher surface brightness, indicative of a concentrated galactic nucleus. Fainter, diffuse light extends outwards from the center, fading into the background. There is minimal evidence of significant tidal disturbances or ongoing mergers, though a subtle asymmetry might suggest a past interaction or minor disturbance. The color profile appears relatively uniform across the galaxy, showing a slight blueish hue near the center with redder features in the halo, suggesting a mix of stellar populations and possible ongoing star formation.
