The galaxy presents as an elliptical morphology with a high degree of central concentration. The light distribution appears smooth and featureless, lacking any distinct spiral arms or prominent dust lanes. The object exhibits a color gradient, transitioning from a bright, nearly white core to a more diffuse, yellowish outer halo. The galaxy appears to be relatively isolated with no nearby interacting companions visible in the immediate field. There are no significant signs of tidal disturbance or ongoing major mergers. Based on its overall appearance, the galaxy is likely a mature system dominated by an older stellar population, with a relatively low current star formation rate. The apparent roundness suggests that it is more of a spherical elliptical (E) rather than a flattened elliptical, although more detailed photometric analysis would be required to confirm this.
