The galaxy presents a somewhat amorphous morphology, exhibiting neither a clearly defined spiral structure nor an elliptical shape. Its color profile suggests a significant population of older stars. The central region appears to be a strong concentration of these stars. The galaxy also has a noticeable irregularity in its form, possibly indicating ongoing or past interaction or merging event(s). Distinct tidal tails or bridges are not readily apparent in the image, though the overall structure does show a disturbed shape that suggests some form of gravitational interaction. The disk is not clearly defined, so its shape must be distorted. The galaxy's overall brightness indicates it's a quite luminous object. There are what appear to be regions of more active star formation scattered around the disk which would suggest the mass is quite large. The galaxy seems to be in a moderately active state of star formation.
