The observed galaxy presents as a disk-shaped structure with a notably bright central bulge. The galaxy's disk exhibits a mottled appearance with hints of spiral arm structures, though these are not sharply defined. A luminous ring-like feature is visible, potentially indicative of ongoing star formation. The color profile suggests the presence of both older stellar populations, contributing to the redder hues in the outer regions, and younger, hotter stars contributing to the bluer tones nearer the core and within the luminous ring. There are faint irregularities observable which suggest minor disturbances, possibly from a recent or ongoing merger event. Overall, this galaxy appears to be a disk galaxy undergoing active star formation.
