The galaxy presents a generally smooth morphology, appearing elliptical in shape, with a high degree of elongation. The central region exhibits a bright, concentrated luminosity, indicating a higher stellar density. A color gradient is visible, with the core appearing redder, potentially indicating an older stellar population. The outer regions show hints of bluer colors, perhaps due to more recent star formation activity. No prominent spiral arms or distinct dust lanes are immediately apparent. There is no indication of any ongoing major merging events, although there is the possibility of a very minor disturbance. The light is slightly redshifted, indicating that it is relatively far away.
