The galaxy presents as a concentrated central object with a largely smooth morphology. Its shape is somewhat elliptical, exhibiting an intermediate roundness rather than appearing distinctly spherical or elongated. The galaxy's color profile suggests the presence of older stellar populations, with a reddish hue dominating the central region, potentially indicating a population of evolved stars and a reduced rate of current star formation. Hints of bluer tones exist on the outer edge of the observed galaxy, though these are less pronounced and may represent a small amount of ongoing star formation. There are no obvious signs of spiral arms or a prominent disk structure; the image is consistent with an early-type galaxy. There appears to be no major merger event happening, but a possible slight disturbance in the galaxy's morphology. 
