The galaxy presents a generally smooth and elliptical morphology. The color profile suggests a relatively older stellar population, concentrated towards the galaxy's center. A subtle color gradient is observable, with the central bulge exhibiting a yellowish hue, transitioning to a slightly bluer tint towards the outer regions. There is a subtle indication of possible faint spiral arms. There are no evident signs of tidal disruption, major mergers, or other significant interactions. Overall, the galaxy appears to be a moderately luminous system, generally consistent with a passively evolving galaxy at moderate redshift.
