The galaxy presents as a relatively smooth, elliptical morphology. The galaxy's light profile appears centrally concentrated, with a gradual decrease in surface brightness towards its outer regions. The color distribution suggests a dominant older stellar population, as indicated by the redder hue in the central bulge, likely consisting of evolved stars. There's a hint of bluer color present in the extended disk, hinting at ongoing star formation, though less intense compared to typical spiral galaxies. The overall structure appears undisturbed, with no significant tidal features or signs of recent mergers visible in this image. The galaxy appears moderately inclined to our line of sight, presenting an elongated, cigar-like shape.
