The galaxy presents as a relatively small, edge-on spiral or lenticular galaxy. Its morphology suggests a notable central bulge, appearing somewhat rounded and concentrated. The galaxy displays a subtle color gradient, with the bulge exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. Fainter, bluish extensions are visible along the major axis, which may represent the disk component, and are suggestive of more recent star formation. These extended features are quite faint, indicating the star formation rate is relatively low. There is no visible sign of any major merger events or significant tidal disturbances. The galaxy appears relatively isolated, with no obvious signs of interactions with neighboring galaxies.
