The galaxy presents as an elliptical morphology with a high degree of central concentration. The light distribution appears relatively smooth, with a noticeable absence of prominent spiral arms or distinct substructures. The core region exhibits a yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, the colour profile shifts towards slightly greener tones, potentially indicating the presence of a younger stellar population or regions of ongoing star formation, although not evidently. The galaxy does not appear to be undergoing any major merging events or tidal disturbances. The object has a subtle, cigar-like shape, that can be seen with careful observation. Overall, the galaxy is an elliptical galaxy with a relatively smooth light distribution.