This galaxy presents a generally smooth morphology, although some subtle features are present, indicating a potential ongoing interaction or internal structure. The overall shape appears somewhat elongated, possibly transitioning from a spheroid to a more cigar-like form. The galaxy exhibits a central concentration of light, suggesting the presence of a prominent bulge or nucleus. The color profile appears relatively uniform, with a slight shift towards redder wavelengths. This redder hue could indicate an older stellar population or significant dust obscuration within the galaxy. There is some indication of a minor disturbance in the upper region of the galaxy, but this is not definitive. This galaxy has a redshift that places it at a significant distance.
