The galaxy presents as a moderately inclined disk. A central bulge appears elongated along the major axis of the disk. There is a moderate amount of internal structure visible, appearing somewhat smooth and indistinct. The color profile appears yellowish with hints of bluer regions likely indicating some regions of star formation, although overall the object has a redder hue, suggesting an older stellar population. The galaxy is fairly compact, with a defined edge despite a slight fuzziness, characteristic of a significant spheroidal component. There is some evidence of minor disturbances in the disk possibly caused by a past minor merger event.
