The galaxy presents an elliptical morphology, elongated along its major axis. Its color profile transitions from a concentrated yellowish hue at the core to a fainter, bluish tint towards the outer edges. No prominent spiral arms or distinct morphological features are discernible, suggesting a relatively smooth and evolved structure. There is a subtle indication of some minor disturbance in the overall morphology, which could potentially be caused by a weak interaction, though it is faint. The light distribution is centrally concentrated, indicative of a relatively old stellar population.