The observed galaxy presents as a relatively bright, elongated structure, exhibiting a general smoothness in its overall light distribution. A dominant central bulge, characterized by a yellowish-white hue, is clearly discernable. This central region appears more concentrated and featureless. Emanating from the bulge, a flattened disk component is observed. The disk appears to be viewed at an oblique angle, giving it a cigar-like shape. There is some subtle color variation within the disk; it transitions from the yellow-white hue near the central bulge to a faint bluish tint further out. This may suggest the presence of younger stellar populations in the outer regions of the galaxy. Additionally, there is an indication of minor disturbances or interactions occurring within the system, evidenced by a possible tidal feature or dwarf galaxy in the lower portion of the image. This small disturbance is bluer in color than the main galaxy. There are no well-defined spiral arms visible.
