The galaxy presents a generally smooth appearance, suggesting a lack of prominent spiral arms or irregular structures. The light distribution is centrally concentrated with an elliptical morphology, exhibiting a relatively high degree of roundness. There is a color gradient with the central region appearing more yellow/orange, indicative of an older stellar population, while the outer regions show a slight hint of blue/green, possibly indicating the presence of some younger stars or ongoing star formation, though not particularly vigorous. No obvious signs of tidal disturbances, major mergers, or strong interactions are observed.
