The galaxy presents as an elongated, somewhat cigar-shaped structure. The light profile suggests a central bulge with evidence of a disk component. There appear to be potential signs of some disturbances within the galaxy, with the bulge having a yellowish tint and with pockets of bright orange star forming regions in the disk. The overall color suggests a relatively older stellar population with on-going star formation. It's is not clear to tell if the star forming regions are from a major merging event or from a minor disturbance.
