The galaxy presents as a smooth, elliptical structure. It has a noticeable central bulge with a yellow-orange hue, suggesting an older stellar population. The light distribution transitions smoothly from the core outwards, lacking prominent spiral arm features. The galaxy appears somewhat elongated, with an apparent cigar-like shape. There is a slight bluer tinge in the outer regions, possibly indicating some level of on-going, albeit subdued, star formation. The overall morphology suggests a system that has largely completed its major assembly, and is in a relatively quiescent state. There is no obvious evidence of a recent major merger or strong tidal interaction.
