The galaxy presents as a somewhat amorphous, albeit concentrated, distribution of luminous material. There appears to be a slight elongation to the structure, suggesting it may be an elliptical galaxy, but without a clear disk morphology. The central region is noticeably brighter and exhibits a distinct greenish-yellow hue, indicating a concentration of intermediate-aged to younger stars and ionized gas. Fainter luminosity extends outwards from the center, forming a more diffuse halo or envelope. There's a suggestion of some internal structure or irregularities within the brighter region, but the resolution is insufficient to determine if these are spiral arms, dust lanes, or some other feature. The overall appearance suggests a galaxy that is relatively quiescent in terms of star formation, but still retains some star-forming capacity.
