The galaxy appears as a somewhat elongated, diffuse object with a smooth, largely featureless morphology. The light is concentrated towards the center, suggesting a prominent galactic nucleus. The color profile indicates a higher concentration of light in the blue end of the spectrum towards the central region, transitioning to redder hues in the outer areas. This could signify a differential stellar population distribution, with younger, bluer stars more prevalent in the core and older, redder stars dominating the periphery. There are no apparent spiral arms or significant dust lanes visible. The overall structure suggests a possible elliptical or lenticular galaxy type, displaying an intermediate level of roundness. There is a hint of minor asymmetry in the outer regions of the galaxy, although this could be related to image noise or minor tidal disturbances. Based on the observed morphology, the galaxy seems relatively isolated with no indication of a major merger event. 
