The galaxy presents as a relatively smooth, elliptical form. There is a clear central bulge that appears bright and concentrated, possibly indicating a high density of older stars. Moving outward from the center, the luminosity decreases gradually. The galaxy appears elongated, with a cigar-like shape. There is no obvious presence of spiral arms, dust lanes, or intense star-forming regions. Color gradients suggest a population shift from a more yellow/white core to a slightly bluer halo, potentially indicating ongoing, albeit mild, star formation in the outer regions, or a population of younger stars. No significant tidal disturbances or signs of a major merger event are apparent, suggesting a relatively isolated and undisturbed evolution.
