The galaxy appears as a relatively compact object with a somewhat smooth morphology. It exhibits a central, brighter core that gradually fades outwards. There is a suggestion of a slight elongation, but no distinct spiral arms or bar structures are readily apparent. The galaxy's color profile indicates a subtle difference between the core and outer regions, with the core potentially showing bluer colors in comparison to the more redshifted outer regions. This could be due to recent star formation within the core or differing stellar populations. There is evidence of some disturbed structure that may be indicative of a potential merger or interaction with another galaxy, though the disturbance is not significantly pronounced. Overall, this galaxy appears to be an elliptical or lenticular type with a possible interaction. Further analysis is required to determine the precise nature of the disturbances and color variations.
