This galaxy appears to be a relatively faint, moderately sized system. The morphology suggests a disk-like structure with some disturbances.  The central bulge is not very pronounced, and there is a suggestion of some spiral arm structure.  The color profile indicates on-going star formation, with bluer regions possibly indicating younger stellar populations. The galaxy exhibits a moderate degree of smoothness in its light distribution, but also shows some signs of more complex features which could be evidence of a past merger or interaction. The overall shape is somewhere between round and elliptical. Some disturbances are visible, although major disruption is not evident.
