The galaxy presents a flattened, elongated morphology, consistent with a disk or cigar-like shape when viewed from this angle. The light is concentrated towards the center, which appears smooth and relatively featureless. The color gradient transitions from a yellowish hue in the central region to a slightly bluer tinge at the outer edges, indicating that star formation is more intense in those areas. The galaxy lacks any obvious spiral arm structures or prominent dust lanes. No signs of tidal tails or major distortions are visible, suggesting that this galaxy has not undergone a recent major merger event, although it displays signs of minor disturbances. The smooth and concentrated light distribution in the central region is characteristic of a substantial bulge component. The estimated physical size suggests that this is a galaxy of significant stature.
