The galaxy presents as a single, largely homogenous object with a generally smooth morphology. The light distribution is concentrated toward the center, with a decrease in intensity towards the outer regions. There is no apparent spiral arm structure or strong disk-like features. The overall shape approximates a circular or slightly elliptical profile, exhibiting a high degree of roundness. The color appears slightly more yellow/red than blue, which is an indication of an older stellar population and diminished star formation activity. There are no readily apparent signs of ongoing or recent merger events, significant tidal disturbances, or major structural irregularities. Based on its appearance, the galaxy is most likely a large and well developed system.
