The galaxy presents a generally elliptical morphology, appearing as a diffuse, elongated structure. The central region exhibits a bright, concentrated luminosity, indicative of a prominent galactic nucleus. Moving outward from the center, the luminosity gradually decreases, though some irregular patches of brightness are observed, hinting at possible internal structures or regions of enhanced star formation. The overall color profile seems to lean toward the redder end of the spectrum, which would align with an older stellar population, as corroborated by the absence of strong spiral arm structures, which are characteristic of younger galaxies. There is also a slight irregular shape. Some faint dust lanes are possibly visible, especially in the outer regions, contributing to the galaxy's slightly mottled appearance. The structure and color suggest that we are observing this galaxy at a relatively late stage in its evolution.