The galaxy presents a generally smooth and rounded morphology. There are no obvious spiral arms or bar structures discernible in this image. The light is concentrated toward the center of the galaxy, with a gradual decrease in intensity towards the outer edges. The color profile suggests a mixture of stellar populations, with the central region showing a slightly blueish tint. This may indicate the presence of younger, hotter stars. The outer regions appear to be dominated by an older stellar population, as indicated by the redder hues. There is a possibility of a merger in its past due to the somewhat disturbed structure in the outskirts of the galaxy, but it is not currently undergoing any major interactions. The relatively small size of the galaxy suggests a lower mass galaxy. There are no noticeable dust lanes or other signs of significant interstellar medium within this galaxy.
