The galaxy presents as a generally smooth and moderately concentrated light distribution, with a slight elongation in its shape. Its color profile appears relatively homogenous, with a faint yellowish-white hue indicating a possible older stellar population. There is no visible spiral structure, prominent dust lanes, or signs of active star formation apparent in this image. The galaxy's morphology suggests a classification towards the elliptical or lenticular type, potentially a galaxy that has undergone significant evolutionary processes. There appears to be no presence of a strong tidal disruption. The galaxy looks undisturbed, based on the available data.
