The galaxy appears to be a relatively compact system with a noticeable central bulge. There is a disk component to the galaxy, although its features are not highly defined. The galaxy exhibits an overall elliptical shape when taking into account the general shape of the disk, with what seems to be an inclination towards our line of sight. Light distribution seems to be smooth across the galaxy's body, with increased luminosity emanating from its central region and fading outwards. A faint halo might be present, but it could simply be background light. There are potential signs of minor disturbances in its shape, perhaps indicating early-stage interactions or the presence of low-level tidal features. However, a significant portion of the light in the surrounding areas may be artifacts from processing. There are no apparent indications of significant merging events.
