The galaxy presents as a lenticular or possibly an elliptical galaxy, based on its morphology. It appears elongated, with a cigar-like shape, suggesting a considerable ellipticity. The galaxy exhibits a smooth, relatively featureless light distribution, with a concentration of light towards the center, indicating a prominent bulge or core. There is no clear evidence of spiral arms or significant dust lanes within the visible light spectrum. The galaxy displays a blue-white hue, potentially suggesting ongoing star formation or a population of relatively young stars, although the smooth appearance is more characteristic of galaxies where star formation has largely ceased. There's no indication of any major merger activity or strong tidal disturbances in the immediate vicinity.
