The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing a warm yellowish hue, which likely indicates an older stellar population. There's a discernible, though subtle, flattening of the overall galactic structure. The light appears to gradually fade from the center outwards, with a lack of distinct features such as spiral arms or prominent dust lanes. There is no evident distortion suggesting an ongoing major merger event, but there is some suggestion of a minor disturbance in the overall structure. The galaxy exhibits a slight elongation, deviating from a perfectly circular appearance.
