The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, with a central concentration that gradually fades toward the outer edges. There is subtle color variation across the galaxy; the core exhibits a slightly yellower hue, possibly indicative of an older stellar population, whereas the outer regions appear marginally bluer. These bluer regions may indicate areas of more recent star formation. There is no obvious spiral structure or distinct disk features visible. Based on the overall appearance, this galaxy is likely an elliptical galaxy or a lenticular galaxy viewed edge-on. There is no obvious sign of any major disturbances or ongoing merging events. The galaxy appears relatively isolated and undisturbed in this field of view.
