The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. The central region exhibits a concentrated, bright core, with a gradual decrease in luminosity towards the outer edges. The color profile appears to be redder in the core, indicating a population of older stars. A faint, blue-ish extension is visible at one end of the galaxy, which could be an area of increased star formation. There are no visible spiral arms or distinct dust lanes. Overall, the galaxy shows no strong signs of any major ongoing mergers. There are no rings or bar features, and the galaxy does not appear to be a perfect ellipse.
