The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type. The light is concentrated in a central bulge, surrounded by a more diffuse halo. There is a slight elongation suggesting an elliptical shape, but it isn't extremely cigar-shaped. The color profile indicates the presence of older stellar populations, showing a yellowish/reddish hue in the central regions. Faint hints of bluer light exist within the outer regions, suggesting there may still be some low-level star formation. No prominent spiral arms or dust lanes are observed. No major signs of a recent or ongoing merger.
