The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core region displays a brighter, somewhat reddish hue, transitioning to a surrounding halo of greenish-white light. There is little evidence of distinct spiral arms or a well-defined disk structure. The galaxy's shape seems roughly circular, exhibiting a moderate degree of roundness without significant elongation or distortion. No major merger events or tidal disturbances are immediately apparent in this imagery. There might be slight irregularities in the outer regions, but the overall impression is one of relative uniformity. The observed colors suggest a moderate population of older stars with some ongoing star formation, particularly within the central regions of the galaxy.
