The galaxy presents as a relatively smooth and compact system, appearing elliptical in overall shape. There appears to be a brighter, more concentrated central region with decreasing luminosity outwards towards its edges.

Distinct color gradients are evident across the galaxy. The central region exhibits a yellowish-orange hue, suggesting an older stellar population. Towards the outer regions, a shift towards bluer colors indicates the presence of younger, hotter stars, particularly on the lower half of the image.

There is evidence of possible disturbance or interaction in the galaxy. The overall structure appears slightly asymmetric. Further investigation is required to determine the nature and extent of this morphological irregularity and its potential impact on the galaxy's evolution.
