The galaxy presents as a spiral structure, though the resolution limits a detailed assessment of its arm morphology. A notable feature is the presence of what appears to be a substantial central bulge, though it is difficult to determine its exact size relative to the galactic disk. The color distribution within the galaxy suggests varying stellar populations, with the central region exhibiting a redder hue, potentially indicative of older stars, while the outer regions show bluer tones, suggestive of younger stellar populations or ongoing star formation. There may be a bar feature. Furthermore, there are some visible knots of brighter emission suggesting possible star forming regions, and some distortion of the spiral shape which may indicate recent merger activity. The galaxy overall appears relatively massive and demonstrates ongoing star formation processes.
