This galaxy presents a generally smooth and elongated morphology, appearing as a flattened spheroid rather than a distinct disk. The central region exhibits a slightly brighter, more concentrated luminosity gradient, suggesting a possible nucleus or bulge. The color profile suggests a moderate level of recent or ongoing star formation, contributing to a bluer overall hue. There is a subtle asymmetry or minor disturbance in the galaxy's structure, possibly indicating an interaction or minor merger event. Although the galaxy appears mostly undisturbed, there is evidence for a slightly more elongated morphology rather than spherical.
