The galaxy appears as an elongated, spindle-shaped object. It presents a relatively smooth light distribution with no distinct spiral arm structures or prominent dust lanes visible in this image. The central region exhibits a slightly brighter, yellowish hue suggestive of an older stellar population, potentially a galactic bulge. The outer regions display a fainter, bluer color profile, which may indicate the presence of younger, hotter stars and ongoing star formation. The galaxy's overall morphology suggests it is likely an edge-on spiral or lenticular galaxy viewed from Earth. There are no obvious signs of major mergers or strong tidal distortions, though minor disturbances cannot be ruled out without further spectroscopic analysis.
