The galaxy presents as an elongated, cigar-shaped structure, suggestive of an elliptical morphology or a disk galaxy viewed at a high inclination. It exhibits a smooth, largely featureless appearance. A central concentration of light is observed, implying a bulge component. The color profile appears generally red, indicating an older stellar population and minimal ongoing star formation. Faint blueish regions are possibly present at the outer edges suggesting a recent, low level of star formation activity. There is no evidence of any significant merger activity or major disturbances in the galaxy's structure. The overall impression is of a mature galaxy with characteristics between an elliptical and a highly inclined disk.
