The galaxy appears to be a somewhat smooth, elliptical-like galaxy with a centrally concentrated bulge. There is not a defined disk structure visible. The galaxy exhibits an overall yellowish hue, which could indicate an older stellar population with less ongoing star formation. The galaxy may be interacting with a smaller companion galaxy, as there is a secondary concentration of light slightly offset from the main body. This secondary object appears more reddish in color, which could signify a different stellar population or dust content. There is no clear evidence of strong tidal tails or other significant morphological distortions that would indicate a major ongoing merger event, but there may be some minor disturbances in the overall shape.
