The galaxy presents an overall elliptical morphology, appearing quite smooth and rounded. There is a concentrated central bulge, exhibiting a bright yellowish hue, which may be indicative of an older stellar population. The outer regions of the galaxy are less defined, gradually fading into the background sky. There is minimal evidence of spiral arms or disk-like features. The colour is slightly redder toward the center, and this reddening gradually decreases outwards into the halo. Faint hints of blue appear to be present in the surrounding regions, though these are very subtle. There are no strong signs of ongoing star formation in the visible light wavelengths. The lack of visible dust lanes or significant irregularities suggests it is not currently undergoing a major merger or interaction.
