The galaxy presents as an elongated, cigar-shaped structure, indicating an elliptical morphology. There is a smooth light distribution, with a concentration of light towards the central region, suggesting a bulge. The color gradient transitions from a slightly redder hue at the center to bluer tones in the outer regions. This may imply that the outer regions have younger stars and/or lower metallicity. There are no easily discernible spiral arms or prominent dust lanes, further supporting the classification of an elliptical galaxy. There is no major signs of disturbance or ongoing merging events.
