The galaxy presents as a relatively compact object, exhibiting a flattened, elliptical morphology rather than a distinct spiral structure. The central region of the galaxy is characterized by a bright, concentrated luminosity, suggesting a dense stellar population within the galactic nucleus. Moving outwards, the light intensity gradually decreases, forming a diffuse halo surrounding the core. While no prominent spiral arms or bar features are visible, there are some slight asymmetries in the outer regions, possibly indicating minor disturbances or past interactions. The color distribution across the galaxy appears relatively uniform, dominated by bluer wavelengths with hints of a yellow hue, with no concentrated red areas, indicating a mix of stellar populations, with a rate of star formation slightly less than one solar mass per year.
