The galaxy presents as a relatively bright, smooth object with an elliptical morphology. A distinct central bulge dominates the structure, characterized by a yellowish-orange hue. This coloration suggests an older stellar population, potentially dominated by red giants and stars nearing the end of their life cycle.

The galaxy exhibits a noticeable flattening, transitioning from the bright center outwards. There is limited visible structure such as spiral arms or dust lanes. The shape suggests a slightly elongated form, not perfectly spherical, leaning towards a cigar shape. There are subtle, diffuse extensions that suggest a faint halo surrounding the main body of the galaxy. No significant tidal features or signs of ongoing major mergers are immediately apparent, but some slight asymmetry may hint at minor gravitational interactions. The light emitted is generally redder in colour, typical of a galaxy with a small number of young stars.
