The galaxy presents a generally smooth, elliptical morphology, appearing approximately 15,000 light years in diameter. It exhibits a slightly elongated, cigar-like shape. The central bulge displays a concentrated brightness and exhibits a yellowish-white hue, suggesting a population of older stars. There are hints of some minor disturbances in the outskirts, but no obvious signs of a major ongoing merger, however there is some presence of star forming activity. The overall structure indicates a relatively evolved system.
