The galaxy presents as an elliptical morphology, approximately cigar-shaped in appearance. The central region exhibits a bright, concentrated nucleus that fades gradually towards the outer edges of the galaxy. The color profile shows a yellowish hue in the core, suggesting an older stellar population with fewer young, massive stars, possibly indicating minimal active star formation. The overall structure appears relatively smooth, lacking prominent spiral arms or distinct dust lanes. There is a slight elongation along a specific axis, suggesting some degree of flattening. A subtle change in color is observable from the center towards the edge, possibly related to variations in stellar populations or dust content. The galaxy does not show obvious signs of recent major mergers or significant tidal disturbances.
