The galaxy presents as an elongated, disk-shaped structure, with an apparent red-shift giving it an orange hue. It exhibits a relatively smooth texture throughout, with a slightly brighter, more concentrated core region. Faint extensions or tidal tails are not apparent in this image. The overall morphology suggests an elliptical to early-type spiral classification, without significant dust lanes or spiral arm features visible. The galaxy appears relatively isolated, without obvious signs of recent or ongoing major mergers, although minor disturbances cannot be ruled out given the image resolution. The dominant color implies a stellar population that is mostly older, with a low star formation rate. The compact size of the galaxy indicates it may be a dwarf elliptical or a spiral galaxy seen edge-on from a great distance.
