The galaxy appears to be a relatively massive system, exhibiting a predominantly smooth morphology with a central bulge that dominates the overall light profile. The bulge component appears yellowish, suggesting an older stellar population. There's a faint disk component with some evidence of structure, though it isn't as clearly defined as in spiral galaxies. It's likely somewhere in between round and in between.

There are hints of bluer regions in the outer parts of the disk which implies some on-going star formation. No signs of tidal tails or other major merger signatures are visible, although there may be minor disturbances within the disk. It could be a possible lenticular galaxy viewed at a slight angle.
