The galaxy exhibits a generally smooth morphology. It appears as an elongated, somewhat cigar-shaped structure. A central bulge region is visible, characterized by a concentrated, brighter light profile, possibly indicating a higher density of older stellar populations. Surrounding the bulge is a fainter, more diffuse disk component. There is a subtle color gradient, with the central region appearing slightly redder than the outer regions, suggesting a difference in stellar populations or dust content. The disk exhibits some subtle irregularities, which could indicate minor disturbances, perhaps due to past interactions or internal processes. There are no prominent spiral arms or a well-defined disk structure visible.
