The galaxy presents a largely smooth morphology, indicating a well-evolved system. It exhibits a distinctly elliptical shape, with a significantly elongated structure, appearing nearly cigar-shaped in its overall form. A concentration of light is observed toward the galaxy's center, suggesting the presence of a substantial galactic bulge or a supermassive black hole in an inactive phase. The galaxy's color profile displays a yellowish-orange hue within its central region, with a slight bluer tinge towards its outer edges. This color gradient likely indicates a population of older stars dominating the core, transitioning to younger stars with ongoing, albeit subdued, star formation in the outer regions. There is no visible evidence of spiral arms or prominent dust lanes. The galaxy appears to be relatively isolated, showing no strong signs of ongoing or recent merger activity or major disturbances in its structure.
