The galaxy presents as a smooth, elliptical structure with a high degree of central concentration. The light distribution exhibits a gradual decline from the core outwards, suggesting an older stellar population. The galaxy shows a slightly elongated shape, potentially indicating it's a barred spiral or undergoing a minor tidal disturbance, though there is no clear visual evidence of distinct spiral arms or a prominent bar in the image. There is little evidence of dust lanes or recent star formation, aligning with the description of a predominantly smooth morphology. The color appears generally blue, with redder components, indicating a mixture of stellar populations. The object does not exhibit any obvious signs of a major merger. It appears that the galaxy has a large amount of neutral hydrogen.
