The galaxy presents a generally smooth and rounded morphology. It appears elliptical, exhibiting a radial gradient of luminosity, with a bright, concentrated core gradually fading into a fainter, extended halo. Color gradients are subtle, with the central region exhibiting a slightly yellower hue suggestive of older stellar populations, transitioning to a marginally bluer color in the outer regions. There are no prominent spiral arms or distinct dust lanes visible, indicating a lack of significant ongoing star formation activity. The overall structure appears largely undisturbed, with no signs of major tidal interactions or ongoing mergers. A slight asymmetry or minor disturbance in the halo, potentially related to a past interaction is visible upon inspection.
