The galaxy presents a mostly smooth morphology. It has a centrally concentrated, spheroidal appearance, suggesting it is likely an elliptical or S0 type. The light distribution is relatively even across the galaxy's body, with a gradual decline in intensity towards the outer regions. There is a slight hint of a possible disk component. The color appears yellowish, indicative of an older stellar population dominated by redder stars. This suggests a lower rate of ongoing star formation. There may be some very minor disturbance in morphology, but overall the galaxy is mostly undisturbed, without clear evidence of a major recent merger. The galaxy's shape is somewhat in-between round and elongated.
