The galaxy presents as a single, moderately luminous object, exhibiting a somewhat elliptical morphology. It appears relatively smooth in structure, with a dominant central bulge and a faint, disk-like extension. The color profile shows a central concentration of light, trending towards a redder hue, suggesting an older stellar population and diminished star formation in that region. The outer regions of the galaxy, while less defined, exhibit a bluer tint implying the presence of younger stars and ongoing star formation. Overall, the galaxy appears to be undergoing, or has undergone, some sort of merging event which is disturbing its morphology.
