The galaxy presents an overall smooth morphology. There is a central bright core, surrounded by a more diffuse region of light. While mostly smooth, a subtle distortion or potential tidal feature is suggested by the slight asymmetry in the surrounding light distribution. There is no clear indication of spiral arms or a well-defined disk structure, and instead, the light appears more spheroidal in nature. The color gradient shows a shift from bluer tones in the inner regions, suggesting younger stellar populations, to redder tones at the outer edges of the galaxy which could be indicative of older stellar populations. This suggests the potential of ongoing or recent star formation. Based on the slight asymmetry, there is a weak indication of a possible minor disturbance, suggesting a potential past or ongoing interaction with another galaxy, but it may also be an artifact of the imaging data. The object is not an obvious merging system based on the overall cohesive appearance.
