The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth and indistinct morphology. The central region appears brighter and more concentrated, suggesting a higher density of stellar populations or possibly an active galactic nucleus, although the image resolution limits definitive determination.

Color gradients are subtle, with a possible trend towards bluer hues at the extreme ends of the major axis and a slightly redder hue in the central bulge. This color differentiation may indicate ongoing or recent star formation in the outer regions, contrasting with older, redder stellar populations dominating the core. There is no visible evidence of prominent spiral arms, bars, or significant dust lanes. The overall appearance suggests the galaxy is either an elliptical galaxy seen edge-on, or a highly inclined disk galaxy with low star formation. There are no clear signs of tidal features or recent merger activity.
