The galaxy presents a smooth, relatively undisturbed morphology. It appears largely elliptical, exhibiting a high degree of roundness with a slight tendency towards a more intermediate shape. The galaxy's color profile suggests a population dominated by older stars, emitting light skewed towards the redder end of the spectrum with hints of yellow. There is no clear evidence of spiral arms or significant dust lanes. The galaxy is a relatively compact object with an estimated effective radius of a few kiloparsecs. It shows no major signs of ongoing or recent mergers, indicating a period of relative isolation and quiescent evolution.
