The galaxy presents as an elongated, cigar-shaped structure, oriented approximately vertically in the image. It exhibits a relatively smooth, featureless appearance, with no distinct spiral arms or prominent bulges visible. The color profile suggests the presence of a stellar population with intermediate to low levels of ongoing star formation, as it is characterized by light with a redder hue than the more active star-forming galaxies that would exhibit more blue-shifted light. There is some evidence of a possible minor disturbance or irregularity within the galaxy's structure. The morphology and color indices suggest the object is likely an elliptical or lenticular galaxy at an intermediate redshift. The galaxy seems to be an isolated galaxy with no signs of a major merger.
