The galaxy presents as a single, moderately bright object with a somewhat diffuse appearance. It displays a generally smooth morphology, although it exhibits some noticeable asymmetry. The light distribution is centrally concentrated, but there is a secondary concentration of luminosity to the left of the center. This secondary peak suggests the possibility of a minor interaction or disturbance. The galaxy's overall shape appears somewhat rounded, though not perfectly circular, hinting at a possible elliptical form. The galaxy's color profile shows a slight shift towards redder wavelengths, suggesting a population of older stars and/or dust obscuration. There is no clear evidence of spiral arms or a prominent disk structure within the visible light. The presence of potential tidal features or more complex structures is difficult to ascertain due to the image resolution.
