The galaxy appears as a single, centrally concentrated object. It displays a roughly elliptical morphology, although some degree of irregularity can be observed in its outer regions. The central area of the galaxy exhibits a bright, concentrated luminosity, potentially indicating a dense stellar population or an active galactic nucleus. The overall color profile suggests a relatively evolved stellar population, as the blue wavelengths are less dominant compared to the redder components. There is subtle evidence of potential interaction or tidal disturbance within the galaxy's halo, although this is a minor feature. The galaxy does not obviously exhibit spiral arm structures or a well-defined disk, implying a more spheroidal or elliptical morphological type.
