The galaxy presents a generally smooth appearance, with a notable lack of distinct spiral arms or a prominent central bulge. It appears to be moderately rounded, though not perfectly spherical. There is a slight elongation in its shape, hinting at a possible transition between a round and a cigar-shaped morphology. The galaxy exhibits a yellowish hue, suggesting a population of older stars and relatively low levels of ongoing star formation. While the main body appears undisturbed, there may be minor perturbations or tidal features indicating a past interaction or potential ongoing merger event. Further investigation is needed to confirm the nature of these subtle features.
