The galaxy presents as a flattened, elongated structure with a discernible central bulge exhibiting a yellowish hue, suggesting a population of older stars. Extending from the central region are fainter, bluish areas suggestive of younger stellar populations and potential star formation activity. The galaxy appears relatively smooth, although some subtle irregularities exist, indicative of possible tidal interactions or internal disturbances. The major axis of the galaxy is significantly larger than the minor axis, giving it a cigar-like appearance. Overall, it is a galaxy with an ordered structure, potentially an elliptical galaxy transitioning towards a more disk-like morphology, or possibly a highly inclined spiral galaxy, although distinct spiral arms are not clearly visible. Its shape could be affected by a possible minor gravitational disturbance.
