The galaxy presents as a cigar-shaped, elongated structure. The central region exhibits a concentrated, bright core which appears smooth and relatively featureless. Extending from the core, the galactic body displays a diffuse, fading halo of light. The color profile suggests a bluer hue throughout, indicating a younger stellar population or ongoing star formation. There appears to be a slight asymmetry in the distribution of light, potentially indicative of a gravitational interaction or past merger event, though the overall structure is largely undisturbed. Based on the morphology, this galaxy is likely an elliptical galaxy.
