The galaxy presents as a cigar-shaped structure. It is likely a lenticular or edge-on spiral galaxy, given the flattened appearance. A central bulge appears prominent with a relatively smooth light distribution suggesting an older stellar population. There appears to be a disk component; however, the viewing angle makes it difficult to resolve any spiral arm structure. Patches of bluer light are interspersed within the galaxy. These are likely regions of active star formation, suggesting ongoing, albeit low-level, stellar birth within the system. There's no obvious evidence of recent or ongoing major merger activity, such as tidal tails or strong asymmetries in the light distribution. The galaxy does not appear to be perfectly smooth. The overall color suggests a mixture of stellar populations.
