The galaxy presents a generally smooth morphology, exhibiting a slightly elongated, intermediate form rather than a perfectly circular or highly elongated shape. A bright central bulge dominates the structure, with light gradually diminishing outwards. Subtle features, possibly faint spiral arms or tidal disturbances, may be present, but are not sharply defined. The galaxy's color profile suggests ongoing star formation. A blue hue is detected, which is concentrated primarily within the central region. This color could be indicative of a population of younger, hotter stars and ongoing star formation activity. Based on the faint asymmetry, this galaxy is likely undergoing a minor interaction with another nearby object.
