The galaxy presents a primarily smooth morphology. The shape is generally rounded, exhibiting a slight elongation, with no distinct spiral arm structures visible. The central region displays a concentrated, bright core indicative of a significant stellar population. There is some indication of disturbances within the galaxy. There are signs of possible recent or ongoing interaction/merger with one or more companion galaxies, evidenced by faint streams or tidal features extending from the main body, or perhaps internal asymmetries in the main galaxy's body. The overall color is a reddish-yellow hue, suggesting a population of older stars with less ongoing star formation.
