The galaxy appears to be a relatively smooth, elliptical system, exhibiting a concentrated central bulge that fades gradually into the outer regions. The overall color profile indicates an older stellar population, likely dominated by redder stars. There's no clear evidence of spiral arm structure or significant dust lanes. A slight asymmetry in the outer halo suggests a potential minor tidal interaction or past merger event, although no major disturbances are immediately obvious. The galaxy's round shape suggests that it's either an E0 or E1 type elliptical, however the hint of asymmetry would suggest E2 or E3. The system is most likely not experiencing a high rate of active star formation, but rather seems to be a settled, relatively quiescent galaxy.
