The galaxy presents a somewhat amorphous morphology, appearing largely smooth with a slight elongation. A subtle disk-like structure might be present but is not clearly defined. Its color profile suggests an older stellar population, with a dominant redder hue at the core that fades to a slightly bluer color toward the outer regions. There is an indication of a potential interaction or minor disturbance exhibited in the non-uniform light distribution. No prominent spiral arms or bar structures are discernible. It exhibits a moderately compact appearance, without signs of significant recent star formation.
