The galaxy presents as a relatively smooth, elliptical structure. Its morphology is generally regular, with a noticeable elongation, trending towards a cigar shape. There is a central concentration of light, indicative of a possible bulge. The light profile appears diffuse, lacking sharp boundaries, suggesting a gradual decrease in stellar density from the core to the outer regions. The color profile shows a generally redder hue, with a slight shift towards bluer tones further from the center. This may indicate that the outer regions have lower star formation rates than the center. There is no evident sign of spiral arms, bars, or any significant tidal disturbances or mergers in progress.
