The galaxy presents a largely smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. There is a subtle color gradient, with the core being slightly more yellow and the outer regions showing hints of a bluer tint. The galaxy lacks any distinct spiral arm structure or prominent dust lanes, further supporting its classification as an elliptical. There is no signs of any active merging, though some tidal disturbances could be occuring within the outer regions. The galaxy appears to be fairly isolated in the image, with no nearby galaxies appearing to strongly influence its structure.
