The galaxy presents an overall smooth morphology. The light distribution appears relatively uniform, exhibiting a mostly featureless structure. There is a slight elongation in the galaxy's shape, appearing somewhere between round and cigar shaped, with a dominant "in between" shape. A hint of a possible disk structure is visible, but indistinct. There may be a minor disturbance from a possible merger event, perhaps with some tidal streams. The central region of the galaxy exhibits a brighter, more concentrated area, indicating a possible galactic nucleus. The color profile exhibits a noticeable trend, with the core of the galaxy showing a shift toward the blue end of the spectrum. This bluer hue contrasts with the outer regions of the galaxy, which present a more reddish tone. This may be due to differing stellar populations and ongoing star formation in the central area. The apparent size of the galaxy is moderate.