The galaxy presents as an elliptical morphology, displaying a smooth and largely featureless structure. The light distribution is centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. The core exhibits a yellowish hue, potentially indicating an older stellar population. There are no apparent spiral arm structures or significant dust lanes visible in this image. The overall shape is generally rounded, with a slight elongation, suggesting it is not perfectly spherical. There is no apparent sign of any major ongoing merger event, though some minor structural disturbances cannot be ruled out at this resolution. The galaxy has an estimated extent of approximately 5 kpc.
