The observed galaxy presents as a relatively small, luminous object. Its overall shape is elliptical, appearing largely smooth and round. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. Faint suggestion of a flattened disk morphology. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal disruptions. There is a small, low luminosity portion that suggests minor disturbances. It exhibits a general blue tint, which may indicate presence of relatively young stellar populations or ongoing star formation activity. Overall, the galaxy presents morphological characteristics consistent with an early-type galaxy, though with minor disturbances or blue features that require further study.
