The galaxy presents as a relatively compact object, displaying a slightly elongated, though mostly rounded, morphology. A significant portion of the galaxy's light appears to be concentrated in a central region, suggestive of a prominent galactic bulge. There are no well-defined spiral arm structures immediately evident. However, faint irregularities in the outer regions may indicate the presence of subtle disk-like features or potential tidal disturbances. The color profile suggests the galaxy is primarily composed of older stellar populations. There is a potential indication of a minor interaction or disturbance within the galaxy's structure, although this is only weakly suggested from the data available in the image.
