The galaxy appears as two distinct components: a central, brighter, and more circular region, and a dimmer, more extended region that is offset from the center. The brighter region exhibits a bluish-white hue, suggesting a population of relatively young, hot stars, as is characteristic of star-forming areas. In contrast, the dimmer region is yellower in color, which is indicative of a population of older, redder stars. The overall light profile of the galaxy is relatively smooth. There appears to be a possible minor disturbance in the morphology with a potential indication of an ongoing or recent merger/tidal interaction causing this offset.
