The object appears to be a relatively smooth, round galaxy, exhibiting characteristics of an elliptical morphology. There is an indication of a very slight tidal disturbance or a possible interaction occurring, but the overall structure is dominated by the smooth, spheroidal component. The color profile suggests an older stellar population with the presence of some intermediate-age stars, indicated by the yellowish hue. There is also a significant presence of dust, obscuring the blue light. No distinct spiral arms or prominent features are apparent. The luminosity profile seems centrally concentrated with a relatively low rate of star formation. It could possibly be undergoing a minor merger event.
