The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. It has a moderately round shape, with subtle hints of elongation along a horizontal axis. The color profile suggests a dominant population of older stars, reflected in the reddish-yellow hue of the central bulge. There is faint evidence of bluer components on the edges of the object suggesting on-going star formation. No spiral arms are readily apparent. There may be some minor gravitational disturbance, but the galaxy's overall structure is generally undisturbed.
