The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with light appearing relatively uniform and decreasing gradually with radial distance. The light profile indicates an absence of distinct spiral arms or bar structures. There is a slight bluing in some parts of the object, indicating star formation is present in the galaxy. There are no obvious signs of tidal disturbance or major merger activity, although subtle irregularities cannot be ruled out at this resolution. The galaxy's color suggests a stellar population of moderate age.
