The galaxy presents as a somewhat elongated or cigar-shaped structure. The light distribution suggests a dominant central bulge component, exhibiting a smooth, concentrated appearance. This central region appears yellowish-orange in color, indicative of an older stellar population. Fainter, bluer light is observed in the surrounding disk, particularly at the edges, possibly indicating regions of recent star formation, albeit at a relatively low rate. Some slight disturbances are present. This galaxy appears to be a disk galaxy, viewed at an angle.
