The galaxy presents as a relatively smooth, centrally concentrated object. It has an elliptical morphology, appearing slightly elongated. The color profile exhibits a gradient, with the core displaying a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, the color transitions subtly towards redder tones. There are no prominent spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. Some slight disturbances are evident in the light profile, suggestive of possible recent or ongoing interactions.
