The galaxy presents an elongated, somewhat cigar-shaped morphology. It appears relatively smooth with a brighter central bulge and fainter, less defined outer regions. A hint of disklike structure is suggested by the extended, flattened shape, although distinct spiral arms are not visible. Color gradients are present; the central bulge exhibits a yellow-white hue suggesting an older stellar population, while the outer regions show a subtle bluish tint. The apparent lack of significant dust lanes supports the inference of a primarily smooth structure with little ongoing major star formation, although some level of star formation cannot be ruled out given the slight blue color in the outer regions. There's no clear indication of any major merger activity or significant tidal disturbances in its immediate vicinity.
