This galaxy appears to be a relatively smooth, disk-dominated system. It exhibits a central bulge that is yellowish-white in color, suggesting an older stellar population. Extending outwards from the bulge is a fainter, more diffuse disk component that displays a bluer hue, indicative of ongoing star formation. There seems to be some disturbance within the galaxy. There is an area that is reddish in hue, suggesting dust lanes or regions of active star formation. Overall, the galaxy is relatively luminous, with the blue color in the disk suggesting a moderately high star formation rate. The galaxy's elongated shape suggests a morphology somewhere between a spherical and a cigar-shaped galaxy.
