The galaxy presents as an elongated, disk-like structure. A centrally concentrated bulge region exhibits a yellow-orange hue, suggestive of an older stellar population and/or significant dust obscuration. Extending outward from the central bulge is a faint, diffuse disk. The disk appears to be tilted with respect to our line of sight. Hints of bluer regions are present within the disk, possibly indicating areas of more recent star formation. Overall, the galaxy appears relatively smooth in texture, lacking prominent spiral arm structures or bright star-forming knots. The galaxy exhibits a slight deviation from a perfectly elliptical shape, leaning towards a cigar shape. There is no evidence of a significant ongoing merger. Some indication of minor disturbance exists, though this is difficult to ascertain.
