This galaxy presents as a somewhat elongated system, exhibiting characteristics of a disk galaxy seen at a high inclination. The central region displays a concentrated, yellowish-white luminosity, suggesting an older stellar population. Extending outwards from this central region, there is a fainter, blueish halo that gradually fades into the background. This blue hue likely indicates the presence of younger, hotter stars and star formation regions. There is a possible irregularity at one end of the galaxy that may indicate tidal disturbance or interaction with another galaxy, although more data is needed to confirm this. The system is not a perfectly smooth elliptical, but neither does it exhibit strong spiral arm structure. It appears to have a moderate rate of star formation. The overall appearance suggests a galaxy undergoing some level of dynamic activity.
