The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly circular morphology, with a bright, prominent core that gradually diffuses outwards into a more indistinct halo. There is little evidence of spiral arm structure or distinct features such as dust lanes within the visible extent of the galaxy. The color appears fairly uniform across the galaxy, with a slight blue tinge particularly around the core, transitioning to a redder hue in the outer regions. This subtle color variation may indicate a population gradient, with younger, bluer stars more concentrated in the center and older, redder stars more prevalent in the outskirts. The overall appearance suggests a possible elliptical galaxy, or perhaps a lenticular galaxy viewed face-on. The lack of significant morphological disturbances implies it is not currently undergoing a major merger, although there is very slight asymmetry indicating a possible minor interaction.
