The galaxy appears to be an elliptical galaxy, seen at a moderate distance. The core region exhibits a high degree of symmetry and concentration of light. There's a smooth decrease in luminosity outwards from the core, with no distinct spiral arms or bar structures visible. The overall shape appears somewhat flattened, hinting at a possible elliptical morphology, but it is difficult to ascertain the exact shape with certainty. The galaxy shows a redder hue, typical of galaxies dominated by older stellar populations. There is no evidence of strong dust lanes or active star formation regions from the image. The galaxy does not appear to be undergoing any major interaction or merging events.
