The galaxy presents an elliptical morphology with a smooth, centrally concentrated light distribution. Its overall shape is elongated, displaying a cigar-like appearance. The galaxy exhibits a color gradient, transitioning from a redder core to bluer outer regions. The core shows a pronounced concentration of older stellar populations which radiates strongly in the redder bands. Conversely, the bluer hues at the periphery suggest the presence of younger, star-forming regions or a more metal-poor stellar population in these areas. There is no apparent evidence of spiral arms, a prominent disk structure, or any major merging events. The galaxy appears to be a relatively isolated system, showing no signs of tidal disturbances or interactions with nearby companions.