The galaxy appears as a relatively smooth, centrally concentrated object. It is primarily bluish in color, suggesting a moderate population of young, hot stars. The overall shape tends towards round, but not perfectly so. No obvious spiral arm structures or distinct features are readily visible. There is no evidence of significant ongoing major merging activity or tidal disturbances, although minor irregularities cannot be ruled out at this resolution. The object seems to be a lenticular or early-type spiral galaxy.
