The observed galaxy presents as a predominantly smooth, elliptical morphology. The central region exhibits a pronounced brightness, suggesting a high concentration of stars. Moving outward from the core, the luminosity gradually decreases. The main body of the galaxy appears mostly featureless, with little evidence of distinct spiral arms or significant dust lanes. A slight elongation is observed, indicating a deviation from a perfectly spherical shape. There may be a hint of a faint, extended halo surrounding the galaxy. Faint irregular structure at one end of the galaxy suggests possible tidal interaction with another galaxy. The color profile is consistent with an older stellar population.
