The observed galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. The central region exhibits a brighter, somewhat indistinct bulge. Faint blue-ish color suggests the presence of some younger stars or ongoing star formation, though this activity appears to be weak relative to the galaxy's mass. The galaxy exhibits a fairly smooth profile, with no distinct spiral arms or other significant features visible. There is no indication of any major ongoing merger activity or significant tidal disturbances in its immediate vicinity. The overall morphology indicates a disk galaxy with a relatively quiescent star formation rate and a high probability of being edge-on.
