The galaxy presents a primarily smooth morphology, with a concentrated central region. The overall shape appears somewhat elliptical, leaning towards a more oblate spheroid than a highly elongated structure. There's a subtle suggestion of a disk-like component, though it is not sharply defined. The color profile exhibits a slight gradient, with the central area showing a bluer hue and the outer regions appearing redder. Indications of some minor disturbances within the galaxy's structure are present, potentially hinting at past or ongoing interactions. However, the overall form remains relatively coherent, suggesting it has either recently undergone or is in the early stages of any merging activity. The color suggests ongoing star formation but it does not appear to be at a high rate.
