The galaxy presents a generally smooth, centralized appearance, with a subtle elongation suggesting a departure from perfect sphericity. The central region exhibits a higher concentration of light, appearing almost luminous with a reddish hue that may indicate an older stellar population, although it could possibly be from redshifting of younger populations. Fainter, bluish tinges extend outward from the central region along the major axis, hinting at the presence of younger stars. The galaxy does appear slightly disrupted, perhaps by an ongoing or recent minor interaction. Overall, the galaxy lacks distinct spiral arms or a prominent disk structure, suggesting a classification leaning towards lenticular or elliptical.