The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arm structures. It exhibits an elliptical or lenticular shape, appearing somewhat elongated rather than perfectly spherical. The color gradient suggests a higher concentration of older stellar populations, particularly towards the core, which is visible in the redder hues observed there.  The outer regions, showing a slightly bluer tint, may indicate some ongoing, though subdued, star formation activity. No signs of strong tidal interactions or major mergers are immediately apparent, although the slight asymmetry of the galaxy's shape could hint at a past minor interaction or disturbance.
