The galaxy presents as a relatively compact, disk-like structure with an overall smooth morphology. The central region exhibits a noticeable concentration of light, suggesting the presence of a bulge or nucleus. Faint spiral arm features can be suspected, though not conclusively observed. The galaxy exhibits a blue hue, suggesting a population of younger, hotter stars and ongoing star formation. There is a potential disturbance in the central region, suggesting a possible merger or close interaction with another galaxy. The galaxy does not appear to be actively undergoing a major merging event. Overall, the galaxy appears to be a relatively evolved spiral or lenticular galaxy, observed at an intermediate redshift.
