The galaxy presents as a centrally concentrated object with a relatively smooth light distribution. It exhibits a slightly elongated morphology, deviating minimally from a perfectly circular shape. There is little evidence of spiral arms or strong features such as dust lanes or bright knots of star formation. The color appears to be trending towards redder hues, indicating an older stellar population and a low rate of on-going star formation. Possible minor disturbance within the galaxy's structure with no major merging events occurring.
