The galaxy presents as a centrally concentrated object with a smooth morphology. The light profile suggests a significant bulge component, with the majority of the light concentrated towards the center. The overall shape appears to be elliptical, exhibiting a slight elongation with an axis ratio that is not perfectly circular but more intermediate. There is a noticeable color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population. Fainter, bluer regions extend outward, indicating the potential presence of some younger stars or ongoing star formation, albeit at a relatively low rate. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's structure. The galaxy does not exhibit any obvious signs of recent major merger activity or significant tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system, likely a massive elliptical galaxy with a mature stellar population and low levels of ongoing star formation.
