The galaxy presents a predominantly smooth appearance, although some subtle features are discernible. Its overall shape appears somewhat elongated, deviating slightly from a perfectly circular morphology. The galaxy's color profile suggests a higher concentration of blue light, indicating the presence of younger, hotter stars. There is a possibility of a minor disturbance within the galaxy's structure, as hinted by a slight asymmetry in the distribution of light. However, there is no obvious evidence of a major merger or significant tidal interactions. Overall, the galaxy exhibits characteristics of a relatively low-mass system with ongoing, albeit modest, star formation activity.
