The galaxy presents an elongated, cigar-shaped morphology. A smooth, centralized bulge is apparent, exhibiting a reddish hue. The outer regions of the galaxy display a bluer tint, suggesting the presence of younger stellar populations or ongoing star formation activity. There is no clear evidence of prominent spiral arms or a well-defined disk structure. Subtle irregularities in the light distribution may indicate minor disturbances. The overall structure suggests this is a relatively evolved galaxy with a significant spheroidal component.
