The galaxy appears as a single, relatively smooth object with a generally elliptical morphology. It presents a concentrated central bulge. There is minimal evidence of distinct spiral arms or bar structure, suggesting a later-type classification. The galaxy exhibits a color gradient, with the core appearing more yellow/red-shifted than the outer regions, suggesting a higher concentration of older stellar populations in the center. The relatively smooth, well-defined structure indicates a galaxy that is not currently undergoing major merger activity or significant tidal disruption. There is a faint, extended halo surrounding the central region. The slight elongation may be due to a minor interaction.
