The galaxy presents a relatively smooth, elliptical morphology. The central bulge is luminous, exhibiting a yellow-orange hue, possibly indicating an older stellar population. Faint, diffuse spiral arms are present and show hints of blue-ish star formation, although the color is less pronounced in the spiral arms, suggesting a lower rate of ongoing star formation. There are indications of disturbances in the galactic structure, potentially indicative of a past merger event, as some features appear irregular and less well-defined.
