The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution and no discernible spiral arm structure. The central region exhibits a higher concentration of light, indicating the likely presence of a galactic bulge. The color profile suggests a stellar population with a relatively low rate of recent star formation, as indicated by the redder hues in the central regions and a fading blue tint further from the core, implying an older stellar population. The galaxy appears undisturbed, lacking any significant tidal features or signs of recent merger activity. The object's shape is mostly in between circular and elliptical, and is mainly smooth, although there is some evidence of minor irregularities and potentially disk-like features along the edge of the galaxy. There may be some minor disturbances, or even features that resemble merging with smaller galaxies.