The galaxy presents as a moderately bright object, appearing as a flattened spheroid with a cigar-like shape. Its central region exhibits a concentrated luminosity, with the overall color suggesting an older stellar population. The galaxy’s profile indicates a relatively smooth structure, with minimal signs of spiral arms or significant dust lanes. There is a subtle color gradient from the core outwards, implying potential variations in stellar populations. The morphological characteristics do not show obvious signs of ongoing or recent major mergers, although minor disturbances cannot be entirely ruled out based on the image alone. The galaxy’s general appearance is consistent with an early-type galaxy at a considerable redshift.
