The galaxy presents as a luminous, centrally concentrated object. Its morphology appears largely smooth, exhibiting a subtle elongation rather than a defined disk structure. The color profile indicates a significant population of older stars, contributing to the galaxy's overall yellowish hue, with slight hints of bluer regions potentially indicating areas of more recent star formation. There is a subtle irregularity to the shape suggesting it might be an intermediate form between elliptical and spiral. There is no evidence of a major ongoing merger event, though subtle asymmetries could imply minor gravitational interactions.
