The galaxy presents as a moderately luminous, elongated structure. The core region appears to be a bright, concentrated spheroid exhibiting a yellowish-white hue, suggesting an older stellar population. Progressing outwards from the central region, the galaxy fades into a less structured disc, with a redder color, potentially indicative of dust obscuration and the presence of younger stars. The overall morphology seems to indicate a possible transition galaxy, between elliptical and spiral type, although definitive spiral arm structures are not visible. There is some evidence of minor disturbance, with possible tidal tails or faint plumes extending from the main body, especially on the bottom end. This could suggest a past or ongoing interaction with another galaxy. The galaxy exhibits a moderate redshift, placing it at a significant cosmological distance.
