The galaxy presents a roughly elliptical morphology, appearing as a flattened disk when viewed from our vantage point. The central region exhibits a bright, concentrated core that gradually diffuses outwards. A distinct ring-like structure surrounds the core, characterized by a blue hue, suggesting the presence of younger, hotter stars and active star formation within this region.

Fainter, diffuse extensions are seen protruding from the main body of the galaxy, indicating possible tidal features or disrupted structures. These extensions show a faint reddish tint, hinting at an older stellar population. There are no distinct spiral arms visible; the overall impression is that of a spheroid with some indications of disturbance or interaction. The smooth appearance of the central region contrasts with the irregular or disturbed nature of the outer structures.
