The galaxy appears as a centrally concentrated, moderately sized elliptical or lenticular system. The central region exhibits a high degree of luminosity, indicating a substantial concentration of stars. Moving outward from the core, the light gradually diminishes, with no distinct spiral arm structures visible in the provided image.

The galaxy displays a generally smooth texture, lacking prominent dust lanes or clumpy star-forming regions. A subtle color gradient might exist, with the central bulge possibly exhibiting a slightly redder hue, suggestive of an older stellar population, while the outer regions may have a marginally bluer color, which could point to a younger stellar population. There is no evidence of tidal tails or significant morphological distortions, suggesting the absence of recent major mergers or strong gravitational interactions with nearby galaxies. The overall shape indicates a moderately elliptical structure, positioned somewhere in between perfectly round and elongated.
