The galaxy appears as an elongated, cigar-shaped structure. There are hints of a disk-like component, though it is not well-defined. The galaxy's light profile suggests it's relatively smooth, with no prominent spiral arms or distinct clumps of star formation readily apparent. The color distribution indicates a primarily older stellar population. The central region shows a slightly yellower hue, potentially indicating a concentration of older stars. Overall, the galaxy seems to be moderately massive. The galaxy appears to have no major ongoing merger events or tidal disturbances.
