The observed galaxy presents an approximately elliptical morphology with a distinct, bright central bulge. The color distribution suggests a possible presence of a substantial old stellar population concentrated within the nucleus. Fainter disk-like structures extend along the major axis, exhibiting a bluer color signature, possibly indicating ongoing star formation. Faint asymmetric extensions are detected from opposite sides of the galaxy, suggesting the potential influence of gravitational interactions or recent minor merging events. Patches of brighter, distinct colors are present on the periphery, suggesting active star forming regions.
