The galaxy presents as a relatively faint, elongated structure. It exhibits a smooth morphology, with no prominent spiral arms or distinct features immediately visible. The light distribution suggests a central concentration of luminosity, possibly indicating a bulge or a bright nucleus. The galaxy displays a colour gradient, appearing bluer towards the outer regions and redder towards the center. The apparent cigar shape is likely a result of its inherent elliptical form, viewed nearly edge on. There is no evidence of any ongoing major mergers or significant tidal disturbances affecting the system based on the single imaging data. The galaxy appears relatively isolated in its immediate environment.