The galaxy appears as a relatively smooth object with a discernible elliptical morphology. Its major axis is significantly longer than its minor axis, indicating a cigar-like shape. A bright, concentrated central bulge dominates the visual structure, exhibiting a yellowish hue, likely indicating an older stellar population. Extending outward from the bulge is a fainter disk, tinged with bluish colors. The disk color suggests the presence of younger, hotter stars and possibly ongoing star formation. No distinct spiral arm structure is readily apparent in this image. There is no clear evidence of a major merger or significant tidal disturbance, though a minor asymmetry cannot be ruled out. The galaxy's overall light profile appears relatively smooth, with the brightness decreasing steadily from the core towards the outer regions.
