The galaxy presents as a relatively smooth, concentrated light distribution. Its overall morphology appears elliptical, lacking prominent spiral arm structures or a distinct disk. The light is concentrated towards the center, indicating a significant central bulge or nucleus. The color gradient suggests a higher proportion of older stellar populations. Based on the colors, we can assume that it has a very low rate of star formation. We can assume that it is a massive galaxy. The slight asymmetry could indicate a minor tidal disturbance or past merger event, but further investigation is needed to confirm such interactions. Overall, the observed characteristics point towards classification as an elliptical or lenticular galaxy, likely with minimal on-going star formation.
