Observed is a galaxy exhibiting a generally smooth morphology, yet appearing slightly disturbed. The galaxy presents an intermediate elliptical shape, leaning toward roundness but not perfectly spherical. A very slight elongation is perceivable, though it's not significantly cigar-shaped. The color profile suggests the presence of an older stellar population, giving it a reddish hue overall. There is no definitive bar structure observed and it is not a spiral galaxy. There are no strong indications of current major merging activity, though minor disturbances may be present suggesting possible interactions or accretion events that has resulted in low levels of star formation within the galaxy.
