The galaxy appears to be a relatively smooth, elliptical system. Its shape is elongated, exhibiting a cigar-like morphology. The central bulge displays a yellowish hue, suggesting a population of older stars. Moving outwards from the center, the color transitions to a slightly bluer tone, hinting at more recent or ongoing star formation in the outer regions. There is no clear evidence of spiral arms or a prominent disk structure. No major disturbances or mergers are apparent, indicating a relatively quiescent evolutionary state.
