The galaxy appears as a relatively smooth, elliptical-shaped object. Its light is concentrated in the center, with the intensity gradually decreasing towards the outer edges, indicative of a bulge. The color profile suggests a higher concentration of older stellar populations, with a slightly redder hue in the outer regions and a bluer tint near the center. The galaxy's shape is somewhat elongated, showing a cigar like or disk shape instead of a sphere. No distinct spiral arms or dust lanes are visible, supporting the observation of a primarily smooth structure. There is little evidence of any major disturbances or merging events, with no apparent tidal tails or asymmetrical features.
