The object presents as a galaxy with a somewhat irregular morphology. The core region exhibits a high surface brightness, appearing bright and compact. There is evidence of an extended disk or arm-like feature to one side of the core. This feature is less defined and shows lower surface brightness than the central bulge. The galaxy does not present a perfectly circular profile, showing an elongated shape suggesting it is not perfectly face on, with some suggestion of an edge on disk. There also appears to be a nearby galaxy interacting with the central galaxy. It is possible there are signs of tidal disruption, possibly indicating an ongoing or past merger event or interaction. The galaxy displays a color gradient, with the central region exhibiting a bluer hue and the outer regions exhibiting a redder hue. This could imply varying stellar populations across the galaxy, with younger, hotter stars concentrated in the center, and older, cooler stars more dominant in the outer parts, but could also be due to dust or other factors.
