The galaxy presents a smooth, elliptical morphology. Its shape appears elongated, with an approximate axis ratio indicating a moderately flattened structure. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges. Color gradients are subtle but present, with a slightly redder hue dominating the core region, transitioning to marginally bluer colors in the outer regions. No distinct spiral arms or prominent dust lanes are discernible. There are no signs of ongoing major mergers, though the galaxy does seem to have minor distrubances. Based on the overall morphology and color profile, it appears to be a relatively massive galaxy with a moderate rate of star formation.
