The galaxy appears as a single, largely homogenous object. It presents with a generally smooth texture and lacks any prominent spiral arms or distinct structural features. The shape tends towards round, exhibiting only a slight ellipticity. There is no obvious major disturbance in its overall structure, suggesting that it has not recently undergone a major merger event. A slight asymmetry may be present on one side, potentially hinting at minor gravitational interaction or a small internal feature. The light profile is centralized, with a gradual decrease in brightness from the core towards the outer edges. The galaxy exhibits a certain degree of homogeneity across its profile.
